센타우루스자리 프록시마 (Korean Wikipedia)

Analysis of information sources in references of the Wikipedia article "센타우루스자리 프록시마" in Korean language version.

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García-Sánchez, J.; Weissman, P. R.; Preston, R. A.; Jones, D. L.; Lestrade, J.-F.; Latham, D. W.; Stefanik, R. P.; Paredes, J. M. (2001). “Stellar encounters with the solar system” (PDF). 《Astronomy and Astrophysics》 379 (2): 634–659. Bibcode:2001A&A...379..634G. doi:10.1051/0004-6361:20011330.

archive.org

See Table 1, Doyle, J. G.; Butler, C. J. (1990). “Optical and infrared photometry of dwarf M and K stars”. 《Astronomy and Astrophysics》 235: 335–339. Bibcode:1990A&A...235..335D. and p. 57, Peebles, P. J. E. (1993). 《Principles of physical cosmology》. Princeton, New Jersey: Princeton University Press. ISBN 978-0-691-01933-8.
Gilster, Paul (2004). 《Centauri dreams: imagining and planning》. Springer. ISBN 978-0-387-00436-5.

arxiv.org

Van Leeuwen, F. (2007). “Validation of the new Hipparcos reduction”. 《Astronomy and Astrophysics》 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357.
Jao, Wei-Chun; Henry, Todd J.; Subasavage, John P.; Winters, Jennifer G.; Gies, Douglas R.; Riedel, Adric R.; Ianna, Philip A. (2014). “The Solar neighborhood. XXXI. Discovery of an unusual red+white dwarf binary at ~25 pc via astrometry and UV imaging”. 《The Astronomical Journal》 147 (1): 21. arXiv:1310.4746. Bibcode:2014AJ....147...21J. doi:10.1088/0004-6256/147/1/21. ISSN 0004-6256.
Benedict, G. Fritz, Chappell DW, Nelan E, Jefferys WH, Van Altena W, Lee J, Cornell D, Shelus PJ (1999). “Interferometric astrometry of Proxima Centauri and Barnard's Star using Hubble Space Telescope fine guidance sensor 3: detection limits for substellar companions”. 《The Astronomical Journal》 118 (2): 1086–1100. arXiv:astro-ph/9905318. Bibcode:1999AJ....118.1086B. doi:10.1086/300975.
Kervella, P.; Thévenin, F.; Lovis, C. (2017). “Proxima's orbit around α Centauri”. 《Astronomy & Astrophysics》 598: L7. arXiv:1611.03495. Bibcode:2017A&A...598L...7K. doi:10.1051/0004-6361/201629930. ISSN 0004-6361. Separation: 3.1, left column of page 3; Orbital period and epoch of periastron: Table 3, right column of page 3.
Ségransan, D.; Kervella, P.; Forveille, T.; Queloz, D. (2003). “First radius measurements of very low mass stars with the VLTI”. 《Astronomy and Astrophysics》 397 (3): L5–L8. arXiv:astro-ph/0211647. Bibcode:2003A&A...397L...5S. doi:10.1051/0004-6361:20021714.
Schlaufman, K. C.; Laughlin, G. (September 2010). “A physically-motivated photometric calibration of M dwarf metallicity”. 《Astronomy and Astrophysics》 519: A105. arXiv:1006.2850. Bibcode:2010A&A...519A.105S. doi:10.1051/0004-6361/201015016.
Passegger, V. M.; Wende-von Berg, S.; Reiners, A. (March 2016). “Fundamental M-dwarf parameters from high-resolution spectra using PHOENIX ACES models. I. Parameter accuracy and benchmark stars”. 《Astronomy & Astrophysics》 587. A19. arXiv:1709.03560. Bibcode:2016A&A...587A..19P. doi:10.1051/0004-6361/201322261. ISSN 0004-6361.
Feng, F.; Jones, H. R. A. (January 2018). “Was Proxima captured by Alpha Centauri A and B?”. 《Monthly Notices of the Royal Astronomical Society》 473 (3): 3185−3189. arXiv:1709.03560. Bibcode:2018MNRAS.473.3185F. doi:10.1093/mnras/stx2576.
Collins, John M.; Jones, Hugh R. A.; Barnes, John R. (June 2017). “Calculations of periodicity from Hα profiles of Proxima Centauri”. 《Astronomy & Astrophysics》 602. A48. arXiv:1608.07834. Bibcode:2017A&A...602A..48C. doi:10.1051/0004-6361/201628827. See section 4: "the vsini is probably less than 0.1 km/s for Proxima Centauri".
Guedel, M.; Audard, M.; Reale, F.; Skinner, S. L.; Linsky, J. L. (2004). “Flares from small to large: X-ray spectroscopy of Proxima Centauri with XMM-Newton”. 《Astronomy and Astrophysics》 416 (2): 713–732. arXiv:astro-ph/0312297. Bibcode:2004A&A...416..713G. doi:10.1051/0004-6361:20031471.
Howard, Ward S.; Tilley, Matt A.; Corbett, Hank; Youngblood, Allison; Loyd, R. O. Parke; Ratzloff, Jeffrey K.; Law, Nicholas M.; Fors, Octavi; Del Ser, Daniel; Shkolnik, Evgenya L.; Ziegler, Carl; Goeke, Erin E.; Pietraallo, Aaron D.; Haislip, Joshua (2018). “The First Naked-eye Superflare Detected from Proxima Centauri”. 《The Astrophysical Journal》 860 (2): L30. arXiv:1804.02001. Bibcode:2018ApJ...860L..30H. doi:10.3847/2041-8213/aacaf3.
Zurlo, A.; Gratton, R.; Mesa, D.; Desidera, S.; Enia, A.; Sahu, K.; Almenara, J. -M.; Kervella, P.; Avenhaus, H.; Girard, J.; Janson, M.; Lagadec, E.; Langlois, M.; Milli, J.; Perrot, C.; Schlieder, J. -E.; Thalmann, C.; Vigan, A.; Giro, E.; Gluck, L.; Ramos, J.; Roux, A. (2018). “The gravitational mass of Proxima Centauri measured with SPHERE from a microlensing event”. 《Monthly Notices of the Royal Astronomical Society》 480 (1): 236. arXiv:1807.01318. Bibcode:2018MNRAS.480..236Z. doi:10.1093/mnras/sty1805.
Benedict, G. F., McArthur, B., Nelan E, Story D, Whipple AL, Shelus PJ, Jefferys WH, Hemenway PD, Franz OG (1998). “Photometry of Proxima Centauri and Barnard's Star using Hubble Space Telescope fine guidance sensor 3: a search for periodic variations”. 《The Astronomical Journal》 116 (1): 429–439. arXiv:astro-ph/9806276. Bibcode:1998AJ....116..429B. doi:10.1086/300420.
Suárez Mascareño, A.; Rebolo, R.; González Hernández, J. I.; Esposito, M. (September 2015). “Rotation periods of late-type dwarf stars from time series high-resolution spectroscopy of chromospheric indicators”. 《Monthly Notices of the Royal Astronomical Society》 452 (3): 2745–2756. arXiv:1506.08039. Bibcode:2015MNRAS.452.2745S. doi:10.1093/mnras/stv1441.
Yadav, Rakesh K.; 외. (December 2016). “Magnetic Cycles in a Dynamo Simulation of Fully Convective M-star Proxima Centauri”. 《The Astrophysical Journal Letters》 833 (2): 6. arXiv:1610.02721. Bibcode:2016ApJ...833L..28Y. doi:10.3847/2041-8213/833/2/L28. L28.
Wood, B. E.; Linsky, J. L.; Müller, H.-R.; Zank, G. P. (2001). “Observational estimates for the mass-loss rates of α Centauri and Proxima Centauri using Hubble Space Telescope Lyα spectra”. 《The Astrophysical Journal》 547 (1): L49–L52. arXiv:astro-ph/0011153. Bibcode:2001ApJ...547L..49W. doi:10.1086/318888.
Cincunegui, C.; Díaz, R. F.; Mauas, P. J. D. (2007). “A possible activity cycle in Proxima Centauri”. 《Astronomy and Astrophysics》 461 (3): 1107–1113. arXiv:astro-ph/0703514. Bibcode:2007A&A...461.1107C. doi:10.1051/0004-6361:20066027.
Wood, B. E.; Linsky, J. L.; Muller, H.-R.; Zank, G. P. (2000). “Observational estimates for the mass-loss rates of Alpha Centauri and Proxima Centauri using Hubble Space Telescope Lyman-alpha spectra”. 《Astrophysical Journal》 537 (2): L49–L52. arXiv:astro-ph/0011153. Bibcode:2000ApJ...537..304W. doi:10.1086/309026.
Lurie, John C.; Henry, Todd J.; Jao, Wei-Chun; Quinn, Samuel N.; Winters, Jennifer G.; Ianna, Philip A.; Koerner, David W.; Riedel, Adric R.; Subasavage, John P. (2014). “The Solar neighborhood. XXXIV. A search for planets orbiting nearby M dwarfs using astrometry”. 《The Astronomical Journal》 148 (5): 91. arXiv:1407.4820. Bibcode:2014AJ....148...91L. doi:10.1088/0004-6256/148/5/91.
Kirkpatrick JD, Davy J, Monet DG, Reid IN, Gizis JE, Liebert J, Burgasser AJ (2001). “Brown dwarf companions to G-type stars. I: Gliese 417B and Gliese 584C”. 《The Astronomical Journal》 121 (6): 3235–3253. arXiv:astro-ph/0103218. Bibcode:2001AJ....121.3235K. doi:10.1086/321085.
Bobylev, V. V. (March 2010). “Searching for stars closely encountering with the solar system”. 《Astronomy Letters》 36 (3): 220–226. arXiv:1003.2160. Bibcode:2010AstL...36..220B. doi:10.1134/S1063773710030060.
Bailer-Jones, C. A. L. (March 2015). “Close encounters of the stellar kind”. 《Astronomy & Astrophysics》 575: 13. arXiv:1412.3648. Bibcode:2015A&A...575A..35B. doi:10.1051/0004-6361/201425221. A35.
Kroupa, Pavel (1995). “The dynamical properties of stellar systems in the Galactic disc”. 《MNRAS》 277 (4): 1507–1521. arXiv:astro-ph/9508084. Bibcode:1995MNRAS.277.1507K. doi:10.1093/mnras/277.4.1507.
Wertheimer, Jeremy G.; Laughlin, Gregory (2006). “Are Proxima and α Centauri gravitationally bound?”. 《The Astronomical Journal》 132 (5): 1995–1997. arXiv:astro-ph/0607401. Bibcode:2006AJ....132.1995W. doi:10.1086/507771.
Johnston, Kathryn V.; Hernquist, Lars; Bolte, Michael (1996). “Fossil signatures of ancient accretion events in the halo”. 《The Astrophysical Journal》 465: 278. arXiv:astro-ph/9602060. Bibcode:1996ApJ...465..278J. doi:10.1086/177418.
Anglada-Escudé, Guillem; Amado, Pedro J.; Barnes, John; Berdiñas, Zaira M.; Butler, R. Paul; Coleman, Gavin A. L.; de la Cueva, Ignacio; Dreizler, Stefan; Endl, Michael; Giesers, Benjamin; Jeffers, Sandra V.; Jenkins, James S.; Jones, Hugh R. A.; Kiraga, Marcin; Kürster, Martin; López-González, Marίa J.; Marvin, Christopher J.; Morales, Nicolás; Morin, Julien; Nelson, Richard P.; Ortiz, José L.; Ofir, Aviv; Paardekooper, Sijme-Jan; Reiners, Ansgar; Rodríguez, Eloy; Rodrίguez-López, Cristina; Sarmiento, Luis F.; Strachan, John P.; Tsapras, Yiannis; Tuomi, Mikko; Zechmeister, Mathias (2016년 8월 25일). “A terrestrial planet candidate in a temperate orbit around Proxima Centauri” (PDF). 《Nature》 536 (7617): 437–440. arXiv:1609.03449. Bibcode:2016Natur.536..437A. doi:10.1038/nature19106. PMID 27558064.
Li, Yiting; 외. (2017년 12월 14일). “A Candidate Transit Event around Proxima Centauri”. 《Research Notes of the AAS》 1 (1). 49. arXiv:1712.04483. Bibcode:2017RNAAS...1...49L. doi:10.3847/2515-5172/aaa0d5.
Bixel, A.; Apai, D. (2017년 2월 21일). “Probabilistic Constraints on the Mass and Composition of Proxima b”. 《The Astrophysical Journal Letters》 836 (2): L31. arXiv:1702.02542. Bibcode:2017ApJ...836L..31W. doi:10.3847/2041-8213/aa5f51. hdl:10150/623234. ISSN 2041-8205.
Endl, M. & Kürster, M. (2008). “Toward detection of terrestrial planets in the habitable zone of our closest neighbor: Proxima Centauri”. 《Astronomy and Astrophysics》 488 (3): 1149–1153. arXiv:0807.1452. Bibcode:2008A&A...488.1149E. doi:10.1051/0004-6361:200810058.
Liu, Hui-Gen; 외. (January 2018). “Searching for the Transit of the Earth-mass Exoplanet Proxima Centauri b in Antarctica: Preliminary Result”. 《The Astronomical Journal》 155 (1): 10. arXiv:1711.07018. Bibcode:2018AJ....155...12L. doi:10.3847/1538-3881/aa9b86. 12.
Kürster, M.; Hatzes, A. P.; Cochran, W. D.; Döbereiner, S.; Dennerl, K.; Endl, M. (1999). “Precise radial velocities of Proxima Centauri. Strong constraints on a substellar companion”. 《Astronomy & Astrophysics Letters》 344: L5–L8. arXiv:astro-ph/9903010. Bibcode:1999A&A...344L...5K.
Lurie, John C.; Henry, Todd J.; Jao, Wei-Chun; Quinn, Samuel N.; Winters, Jennifer G.; Ianna, Philip A.; Koerner, David W.; Riedel, Adric R.; Subasavage, John P. (November 2014). “The Solar Neighborhood. XXXIV. a Search for Planets Orbiting Nearby M Dwarfs Using Astrometry”. 《The Astronomical Journal》 148 (5): 12. arXiv:1407.4820. Bibcode:2014AJ....148...91L. doi:10.1088/0004-6256/148/5/91. 91.
Anglada, Guillem; Amado, Pedro J; Ortiz, Jose L; Gómez, José F; Macías, Enrique; Alberdi, Antxon; Osorio, Mayra; Gómez, José L; Itziar de Gregorio-Monsalvo; Pérez-Torres, Miguel A; Anglada-Escudé, Guillem; Berdiñas, Zaira M; Jenkins, James S; Jimenez-Serra, Izaskun; Lara, Luisa M; López-González, Maria J; López-Puertas, Manuel; Morales, Nicolas; Ribas, Ignasi; Richards, Anita M. S; Rodríguez-López, Cristina; Rodriguez, Eloy (2017). “ALMA Discovery of Dust Belts Around Proxima Centauri”. 《The Astrophysical Journal》 850 (1): L6. arXiv:1711.00578. Bibcode:2017ApJ...850L...6A. doi:10.3847/2041-8213/aa978b.
MacGregor, Meredith A.; 외. (2018). “Detection of a Millimeter Flare From Proxima Centauri”. 《Astrophysical Journal Letters》 855 (1): L2. arXiv:1802.08257. Bibcode:2018ApJ...855L...2M. doi:10.3847/2041-8213/aaad6b.
Endl, M.; Kuerster, M.; Rouesnel, F.; Els, S.; Hatzes, A. P.; Cochran, W. D. (June 18–21, 2002). Deming, Drake, 편집. 《Extrasolar terrestrial planets: can we detect them already?》. 《Conference Proceedings, Scientific Frontiers in Research on Extrasolar Planets》 (Washington, DC). 75–79쪽. arXiv:astro-ph/0208462. Bibcode:2003ASPC..294...75E.
Tarter, Jill C., Mancinelli RL, Aurnou JM, Backman DE, Basri GS, Boss AP, Clarke A, Deming D (2007). “A reappraisal of the habitability of planets around M dwarf stars”. 《Astrobiology》 7 (1): 30–65. arXiv:astro-ph/0609799. Bibcode:2007AsBio...7...30T. doi:10.1089/ast.2006.0124. PMID 17407403.

books.google.com

천정보다 남쪽에 있는 항성이 천정과 이루는 각도는 '위도 − 적위'이다. 항성은 천정과 이루는 각도가 90도 이상일 경우 시야에서 사라진다.(지평선 아래로 내려간다는 뜻임) 센타우루스자리 프록시마의 경우 이 별을 볼 수 있는 최고 위도는
90° + −62.68° = 27.32°이다.
참고: Campbell, William Wallace (1899). 《The elements of practical astronomy》. London: Macmillan. 109–110쪽. 2008년 8월 12일에 확인함.

doi.org

dx.doi.org

Van Leeuwen, F. (2007). “Validation of the new Hipparcos reduction”. 《Astronomy and Astrophysics》 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357.
Jao, Wei-Chun; Henry, Todd J.; Subasavage, John P.; Winters, Jennifer G.; Gies, Douglas R.; Riedel, Adric R.; Ianna, Philip A. (2014). “The Solar neighborhood. XXXI. Discovery of an unusual red+white dwarf binary at ~25 pc via astrometry and UV imaging”. 《The Astronomical Journal》 147 (1): 21. arXiv:1310.4746. Bibcode:2014AJ....147...21J. doi:10.1088/0004-6256/147/1/21. ISSN 0004-6256.
Benedict, G. Fritz, Chappell DW, Nelan E, Jefferys WH, Van Altena W, Lee J, Cornell D, Shelus PJ (1999). “Interferometric astrometry of Proxima Centauri and Barnard's Star using Hubble Space Telescope fine guidance sensor 3: detection limits for substellar companions”. 《The Astronomical Journal》 118 (2): 1086–1100. arXiv:astro-ph/9905318. Bibcode:1999AJ....118.1086B. doi:10.1086/300975.
Kervella, P.; Thévenin, F.; Lovis, C. (2017). “Proxima's orbit around α Centauri”. 《Astronomy & Astrophysics》 598: L7. arXiv:1611.03495. Bibcode:2017A&A...598L...7K. doi:10.1051/0004-6361/201629930. ISSN 0004-6361. Separation: 3.1, left column of page 3; Orbital period and epoch of periastron: Table 3, right column of page 3.
Bessell, M. S. (1991). “The late-M dwarfs”. 《The Astronomical Journal》 101: 662. Bibcode:1991AJ....101..662B. doi:10.1086/115714.
Ségransan, D.; Kervella, P.; Forveille, T.; Queloz, D. (2003). “First radius measurements of very low mass stars with the VLTI”. 《Astronomy and Astrophysics》 397 (3): L5–L8. arXiv:astro-ph/0211647. Bibcode:2003A&A...397L...5S. doi:10.1051/0004-6361:20021714.
Schlaufman, K. C.; Laughlin, G. (September 2010). “A physically-motivated photometric calibration of M dwarf metallicity”. 《Astronomy and Astrophysics》 519: A105. arXiv:1006.2850. Bibcode:2010A&A...519A.105S. doi:10.1051/0004-6361/201015016.
Passegger, V. M.; Wende-von Berg, S.; Reiners, A. (March 2016). “Fundamental M-dwarf parameters from high-resolution spectra using PHOENIX ACES models. I. Parameter accuracy and benchmark stars”. 《Astronomy & Astrophysics》 587. A19. arXiv:1709.03560. Bibcode:2016A&A...587A..19P. doi:10.1051/0004-6361/201322261. ISSN 0004-6361.
Feng, F.; Jones, H. R. A. (January 2018). “Was Proxima captured by Alpha Centauri A and B?”. 《Monthly Notices of the Royal Astronomical Society》 473 (3): 3185−3189. arXiv:1709.03560. Bibcode:2018MNRAS.473.3185F. doi:10.1093/mnras/stx2576.
Collins, John M.; Jones, Hugh R. A.; Barnes, John R. (June 2017). “Calculations of periodicity from Hα profiles of Proxima Centauri”. 《Astronomy & Astrophysics》 602. A48. arXiv:1608.07834. Bibcode:2017A&A...602A..48C. doi:10.1051/0004-6361/201628827. See section 4: "the vsini is probably less than 0.1 km/s for Proxima Centauri".
Alden, Harold L. (1928). “Alpha and Proxima Centauri”. 《Astronomical Journal》 39 (913): 20–23. Bibcode:1928AJ.....39...20A. doi:10.1086/104871.
Voûte, J. (1917). “A 13th magnitude star in Centaurus with the same parallax as α Centauri”. 《Monthly Notices of the Royal Astronomical Society》 77 (9): 650–651. Bibcode:1917MNRAS..77..650V. doi:10.1093/mnras/77.9.650.
Shapley, Harlow (1951). “Proxima Centauri as a flare star”. 《Proceedings of the National Academy of Sciences of the United States of America》 37 (1): 15–18. Bibcode:1951PNAS...37...15S. doi:10.1073/pnas.37.1.15. PMC 1063292. PMID 16588985.
Kroupa, Pavel; Burman, R. R.; Blair, D. G. (1989). “Photometric observations of flares on Proxima Centauri”. 《PASA》 8 (2): 119–122. Bibcode:1989PASAu...8..119K. doi:10.1017/S1323358000023122.
Haisch, Bernhard; Antunes, A.; Schmitt, J. H. M. M. (1995). “Solar-like M-class X-ray flares on Proxima Centauri observed by the ASCA satellite”. 《Science》 268 (5215): 1327–1329. Bibcode:1995Sci...268.1327H. doi:10.1126/science.268.5215.1327. PMID 17778978.
Guedel, M.; Audard, M.; Reale, F.; Skinner, S. L.; Linsky, J. L. (2004). “Flares from small to large: X-ray spectroscopy of Proxima Centauri with XMM-Newton”. 《Astronomy and Astrophysics》 416 (2): 713–732. arXiv:astro-ph/0312297. Bibcode:2004A&A...416..713G. doi:10.1051/0004-6361:20031471.
Howard, Ward S.; Tilley, Matt A.; Corbett, Hank; Youngblood, Allison; Loyd, R. O. Parke; Ratzloff, Jeffrey K.; Law, Nicholas M.; Fors, Octavi; Del Ser, Daniel; Shkolnik, Evgenya L.; Ziegler, Carl; Goeke, Erin E.; Pietraallo, Aaron D.; Haislip, Joshua (2018). “The First Naked-eye Superflare Detected from Proxima Centauri”. 《The Astrophysical Journal》 860 (2): L30. arXiv:1804.02001. Bibcode:2018ApJ...860L..30H. doi:10.3847/2041-8213/aacaf3.
Kamper, K. W.; Wesselink, A. J. (1978). “Alpha and Proxima Centauri”. 《Astronomical Journal》 83: 1653–1659. Bibcode:1978AJ.....83.1653K. doi:10.1086/112378.
Leggett, S. K. (1992). “Infrared colors of low-mass stars”. 《Astrophysical Journal Supplement Series》 82 (1): 351–394, 357. Bibcode:1992ApJS...82..351L. doi:10.1086/191720.
Zurlo, A.; Gratton, R.; Mesa, D.; Desidera, S.; Enia, A.; Sahu, K.; Almenara, J. -M.; Kervella, P.; Avenhaus, H.; Girard, J.; Janson, M.; Lagadec, E.; Langlois, M.; Milli, J.; Perrot, C.; Schlieder, J. -E.; Thalmann, C.; Vigan, A.; Giro, E.; Gluck, L.; Ramos, J.; Roux, A. (2018). “The gravitational mass of Proxima Centauri measured with SPHERE from a microlensing event”. 《Monthly Notices of the Royal Astronomical Society》 480 (1): 236. arXiv:1807.01318. Bibcode:2018MNRAS.480..236Z. doi:10.1093/mnras/sty1805.
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ui.adsabs.harvard.edu

Brown, A. G. A. 외 (2018년 8월). “Gaia Data Release 2. Summary of the contents and survey properties”. 《Astronomy & Astrophysics》 616 (A1): 22. 2020년 2월 11일에 확인함.

chandra.harvard.edu

“Proxima Centauri: the nearest star to the Sun”. Harvard-Smithsonian Center for Astrophysics. 2006년 8월 30일. 2007년 7월 9일에 확인함.

heavens-above.com

“Spacecraft escaping the Solar System”. 《Heavens Above》. 2016년 12월 25일에 확인함.

iau.org

“IAU Working Group on Star Names (WGSN)”. International Astronomical Union. 2016년 5월 22일에 확인함.
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illinois.edu

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inta-csic.es

sdc.cab.inta-csic.es

“Proxima Centauri UV flux distribution”. ESA & The Astronomical Data Centre at CAB. 2007년 7월 11일에 확인함.

nasa.gov

solarsystem.nasa.gov

밀도(ρ)는 질량을 부피로 나눈 값이다. 따라서 태양의 밀도를 이용하여 구한 프록시마의 밀도는 다음과 같다.

$\rho$	= ${\begin{smallmatrix}{\frac {M}{M_{\odot }}}\cdot \left({\frac {R}{R_{\odot }}}\right)^{-3}\cdot \rho _{\odot }\end{smallmatrix}}$
	= 0.122 · 0.154⁻³ · (1.41 × 10³ kg/m³)
	= 33.4 · (1.41 × 10³ kg/m³)
	= 4.71 × 10⁴ kg/m³

이 식에서 ${\begin{smallmatrix}\rho _{\odot }\end{smallmatrix}}$ 는 태양의 평균 밀도이다. 다음 문헌을 참고할 것.

Munsell, Kirk; Smith, Harman; Davis, Phil; Harvey, Samantha (2008년 6월 11일). “Sun: facts & figures”. 《Solar system exploration》. NASA. 2008년 1월 2일에 원본 문서에서 보존된 문서. 2008년 7월 12일에 확인함.

nssdc.gsfc.nasa.gov

Williams, D. R. (2006년 2월 10일). “Moon Fact Sheet”. Lunar & Planetary Science. NASA. 2007년 10월 12일에 확인함.

ntrs.nasa.gov

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nationalgeographic.com

Drake, Nadia (2019년 4월 12일). “A new super-Earth may orbit the star next door”. 《National Geographic》. 2019년 9월 20일에 확인함. Official video of announcement at the 2019 Breakthrough Discuss conference.

nature.com

Witze, Alexandra (2016년 8월 24일). “Earth-sized planet around nearby star is astronomy dream come true”. 《Nature》. 381–382면. Bibcode:2016Natur.536..381W. doi:10.1038/nature.2016.20445. 2016년 8월 24일에 확인함.

newscientist.com

Aron, Jacob. August 24, 2016. Proxima b: Closest Earth-like planet discovered right next door. New Scientist. Retrieved August 24, 2016.

nih.gov

ncbi.nlm.nih.gov

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Anglada-Escudé, Guillem; Amado, Pedro J.; Barnes, John; Berdiñas, Zaira M.; Butler, R. Paul; Coleman, Gavin A. L.; de la Cueva, Ignacio; Dreizler, Stefan; Endl, Michael; Giesers, Benjamin; Jeffers, Sandra V.; Jenkins, James S.; Jones, Hugh R. A.; Kiraga, Marcin; Kürster, Martin; López-González, Marίa J.; Marvin, Christopher J.; Morales, Nicolás; Morin, Julien; Nelson, Richard P.; Ortiz, José L.; Ofir, Aviv; Paardekooper, Sijme-Jan; Reiners, Ansgar; Rodríguez, Eloy; Rodrίguez-López, Cristina; Sarmiento, Luis F.; Strachan, John P.; Tsapras, Yiannis; Tuomi, Mikko; Zechmeister, Mathias (2016년 8월 25일). “A terrestrial planet candidate in a temperate orbit around Proxima Centauri” (PDF). 《Nature》 536 (7617): 437–440. arXiv:1609.03449. Bibcode:2016Natur.536..437A. doi:10.1038/nature19106. PMID 27558064.
Tarter, Jill C., Mancinelli RL, Aurnou JM, Backman DE, Basri GS, Boss AP, Clarke A, Deming D (2007). “A reappraisal of the habitability of planets around M dwarf stars”. 《Astrobiology》 7 (1): 30–65. arXiv:astro-ph/0609799. Bibcode:2007AsBio...7...30T. doi:10.1089/ast.2006.0124. PMID 17407403.
Alpert, Mark (November 2005). “Red star rising”. 《Scientific American》 293 (5): 28. Bibcode:2005SciAm.293e..28A. doi:10.1038/scientificamerican1105-28. PMID 16318021.
Khodachenko, Maxim L., Lammer H, Grießmeier JM, Leitner M, Selsis F, Eiroa C, Hanslmeier A, Biernat HK (2007). “Coronal Mass Ejection (CME) activity of low mass M stars as an important factor for the habitability of terrestrial exoplanets. I. CME impact on expected magnetospheres of earth-like exoplanets in close-in habitable zones”. 《Astrobiology》 7 (1): 167–184. Bibcode:2007AsBio...7..167K. doi:10.1089/ast.2006.0127. PMID 17407406.
Merali, Zeeya (2016년 5월 27일). “Shooting for a star”. 《Science》 352 (6289): 1040–1041. doi:10.1126/science.352.6289.1040. PMID 27230357.
Popkin, Gabriel (2017년 2월 2일). “What it would take to reach the stars”. 《Nature》 542 (7639): 20–22. Bibcode:2017Natur.542...20P. doi:10.1038/542020a. PMID 28150784.

nytimes.com

Chang, Kenneth (2016년 8월 24일). “One star over, a planet that might be another Earth”. 《New York Times》. 2016년 8월 24일에 확인함.

palereddot.org

“Proxima b is our neighbor ... better get used to it!”. 《Pale Red Dot》. 2016년 8월 24일. 2020년 5월 13일에 원본 문서에서 보존된 문서. 2016년 8월 24일에 확인함.

saao.ac.za

Glass, I.S. (2008). 《Proxima, the nearest star (other than the Sun)》. Cape Town: Mons Mensa. 2017년 9월 12일에 원본 문서에서 보존된 문서. 2016년 9월 6일에 확인함.

sciencedaily.com

“Proxima Centauri's no good, very bad day”. 《Science Daily》. 2018년 2월 26일. 2018년 3월 1일에 확인함.

sciencemag.org

advances.sciencemag.org

Damasso, Mario; Del Sordo, Fabio; Anglada-Escudé, Guillem; 외. (2020년 1월 15일). “A low-mass planet candidate orbiting Proxima Centauri at a distance of 1.5 AU”. 《Science Advances》 6 (3). eaax7467. doi:10.1126/sciadv.aax7467.

scientificamerican.com

Billings, Lee (2019년 4월 12일). “A Second Planet May Orbit Earth's Nearest Neighboring Star”. 《Scientific American》. 2019년 4월 12일에 확인함.

si.edu

insider.si.edu

“Proxima Centauri Might Be More Sunlike Than We Thought”. 《Smithsonian Insider》. 2016년 10월 12일. 2016년 11월 2일에 확인함.

space.com

Mathewson, Samantha (2016년 8월 24일). “Proxima b By the Numbers: Possibly Earth-Like World at the Next Star Over”. 《Space.com》. 2016년 8월 25일에 확인함.
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telegraph.co.uk

Knapton, Sarah (2016년 8월 24일). “Proxima b: Alien life could exist on 'second Earth' found orbiting our nearest star in Alpha Centauri system”. 《The Telegraph》 (Telegraph Media Group). 2016년 8월 24일에 확인함.

u-strasbg.fr

simbad.u-strasbg.fr

“SIMBAD query result: V* V645 Cen – Flare Star”. 《SIMBAD》. Centre de Données astronomiques de Strasbourg. 2008년 8월 11일에 확인함. —some of the data is located under "Measurements".

unam.mx

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Adams, Fred C.; Laughlin, Gregory; Graves, Genevieve J. M. 《Red dwarfs and the end of the main sequence》 (PDF). 《Gravitational collapse: from massive stars to planets》 (Revista Mexicana de Astronomía y Astrofísica). 46–49쪽. 2008년 6월 24일에 확인함.

unizar.es

zaguan.unizar.es

Anglada, Guillem; Amado, Pedro J; Ortiz, Jose L; Gómez, José F; Macías, Enrique; Alberdi, Antxon; Osorio, Mayra; Gómez, José L; Itziar de Gregorio-Monsalvo; Pérez-Torres, Miguel A; Anglada-Escudé, Guillem; Berdiñas, Zaira M; Jenkins, James S; Jimenez-Serra, Izaskun; Lara, Luisa M; López-González, Maria J; López-Puertas, Manuel; Morales, Nicolas; Ribas, Ignasi; Richards, Anita M. S; Rodríguez-López, Cristina; Rodriguez, Eloy (2017). “ALMA Discovery of Dust Belts Around Proxima Centauri”. 《The Astrophysical Journal》 850 (1): L6. arXiv:1711.00578. Bibcode:2017ApJ...850L...6A. doi:10.3847/2041-8213/aa978b.

utexas.edu

clyde.as.utexas.edu

Benedict, G. F.; Mcarthur, B.; Nelan, E.; Story, D.; Jefferys, W. H.; Wang, Q.; Shelus, P. J.; Hemenway, P. D.; Mccartney, J.; Van Altena, Wm. F.; Duncombe, R.; Franz, O. G.; Fredrick, L. W. 《Astrometric stability and precision of fine guidance sensor #3: the parallax and proper motion of Proxima Centauri》 (PDF). 《Proceedings of the HST calibration workshop》. 380–384쪽. 2007년 7월 11일에 확인함.

washingtonpost.com

Feltman, Rachel (2016년 8월 24일). “Scientists say they've found a planet orbiting Proxima Centauri, our closest neighbor”. 《The Washington Post》.

web.archive.org

밀도(ρ)는 질량을 부피로 나눈 값이다. 따라서 태양의 밀도를 이용하여 구한 프록시마의 밀도는 다음과 같다.

$\rho$	= ${\begin{smallmatrix}{\frac {M}{M_{\odot }}}\cdot \left({\frac {R}{R_{\odot }}}\right)^{-3}\cdot \rho _{\odot }\end{smallmatrix}}$
	= 0.122 · 0.154⁻³ · (1.41 × 10³ kg/m³)
	= 33.4 · (1.41 × 10³ kg/m³)
	= 4.71 × 10⁴ kg/m³

이 식에서 ${\begin{smallmatrix}\rho _{\odot }\end{smallmatrix}}$ 는 태양의 평균 밀도이다. 다음 문헌을 참고할 것.

Munsell, Kirk; Smith, Harman; Davis, Phil; Harvey, Samantha (2008년 6월 11일). “Sun: facts & figures”. 《Solar system exploration》. NASA. 2008년 1월 2일에 원본 문서에서 보존된 문서. 2008년 7월 12일에 확인함.
Glass, I.S. (2008). 《Proxima, the nearest star (other than the Sun)》. Cape Town: Mons Mensa. 2017년 9월 12일에 원본 문서에서 보존된 문서. 2016년 9월 6일에 확인함.
“Proxima b is our neighbor ... better get used to it!”. 《Pale Red Dot》. 2016년 8월 24일. 2020년 5월 13일에 원본 문서에서 보존된 문서. 2016년 8월 24일에 확인함.

worldcat.org

Jao, Wei-Chun; Henry, Todd J.; Subasavage, John P.; Winters, Jennifer G.; Gies, Douglas R.; Riedel, Adric R.; Ianna, Philip A. (2014). “The Solar neighborhood. XXXI. Discovery of an unusual red+white dwarf binary at ~25 pc via astrometry and UV imaging”. 《The Astronomical Journal》 147 (1): 21. arXiv:1310.4746. Bibcode:2014AJ....147...21J. doi:10.1088/0004-6256/147/1/21. ISSN 0004-6256.
Kervella, P.; Thévenin, F.; Lovis, C. (2017). “Proxima's orbit around α Centauri”. 《Astronomy & Astrophysics》 598: L7. arXiv:1611.03495. Bibcode:2017A&A...598L...7K. doi:10.1051/0004-6361/201629930. ISSN 0004-6361. Separation: 3.1, left column of page 3; Orbital period and epoch of periastron: Table 3, right column of page 3.
Passegger, V. M.; Wende-von Berg, S.; Reiners, A. (March 2016). “Fundamental M-dwarf parameters from high-resolution spectra using PHOENIX ACES models. I. Parameter accuracy and benchmark stars”. 《Astronomy & Astrophysics》 587. A19. arXiv:1709.03560. Bibcode:2016A&A...587A..19P. doi:10.1051/0004-6361/201322261. ISSN 0004-6361.
Bixel, A.; Apai, D. (2017년 2월 21일). “Probabilistic Constraints on the Mass and Composition of Proxima b”. 《The Astrophysical Journal Letters》 836 (2): L31. arXiv:1702.02542. Bibcode:2017ApJ...836L..31W. doi:10.3847/2041-8213/aa5f51. hdl:10150/623234. ISSN 2041-8205.

youtube.com

Drake, Nadia (2019년 4월 12일). “A new super-Earth may orbit the star next door”. 《National Geographic》. 2019년 9월 20일에 확인함. Official video of announcement at the 2019 Breakthrough Discuss conference.

zenodo.org

Voûte, J. (1917). “A 13th magnitude star in Centaurus with the same parallax as α Centauri”. 《Monthly Notices of the Royal Astronomical Society》 77 (9): 650–651. Bibcode:1917MNRAS..77..650V. doi:10.1093/mnras/77.9.650.