Epsilon Eridani (English Wikipedia)

Analysis of information sources in references of the Wikipedia article "Epsilon Eridani" in English language version.

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Soubiran, C.; Jasniewicz, G.; Chemin, L.; Zurbach, C.; Brouillet, N.; Panuzzo, P.; Sartoretti, P.; Katz, D.; Le Campion, J.-F.; Marchal, O.; Hestroffer, D.; Thévenin, F.; Crifo, F.; Udry, S.; Cropper, M.; Seabroke, G.; Viala, Y.; Benson, K.; Blomme, R.; Jean-Antoine, A.; Huckle, H.; Smith, M.; Baker, S. G.; Damerdji, Y.; Dolding, C.; Frémat, Y.; Gosset, E.; Guerrier, A.; Guy, L. P.; Haigron, R.; Janßen, K.; Plum, G.; Fabre, C.; Lasne, Y.; Pailler, F.; Panem, C.; Riclet, F.; Royer, F.; Tauran, G.; Zwitter, T.; Gueguen, A.; Turon, C. (2018). "Gaia Data Release 2". Astronomy & Astrophysics. 616. EDP Sciences: A7. arXiv:1804.09370. Bibcode:2018A&A...616A...7S. doi:10.1051/0004-6361/201832795. ISSN 0004-6361. S2CID 247759802.
Benedict, G. Fritz; et al. (November 2006), "The Extrasolar Planet ɛ Eridani b: Orbit and Mass", The Astronomical Journal, 132 (5): 2206–2218, arXiv:astro-ph/0610247, Bibcode:2006AJ....132.2206B, doi:10.1086/508323, S2CID 18603036.
Gonzalez, G.; Carlson, M. K.; Tobin, R. W. (April 2010), "Parent stars of extrasolar planets – X. Lithium abundances and v sini revisited", Monthly Notices of the Royal Astronomical Society, 403 (3): 1368–1380, arXiv:0912.1621, Bibcode:2010MNRAS.403.1368G, doi:10.1111/j.1365-2966.2009.16195.x, S2CID 118520284. See table 3.
Baines, Ellyn K.; Armstrong, J. Thomas (2011), "Confirming Fundamental Parameters of the Exoplanet Host Star epsilon Eridani Using the Navy Optical Interferometer", The Astrophysical Journal, 748 (1): 72, arXiv:1112.0447, Bibcode:2012ApJ...748...72B, doi:10.1088/0004-637X/748/1/72, S2CID 124270967.
Demory, Brice-Olivier; Ségransan, Damien; Forveille, Thierry; Queloz, Didier; Beuzit, Jean-Luc; Delfosse, Xavier; Di Folco, Emmanuel; Kervella, Pierre; Le Bouquin, Jean-Baptiste; Perrier, Christian; Benisty, Myriam; Duvert, Gilles; Hofmann, Karl-Heinz; Lopez, Bruno; Petrov, Romain (October 2009), "Mass-radius relation of low and very low-mass stars revisited with the VLTI", Astronomy and Astrophysics, 505 (1): 205–215, arXiv:0906.0602, Bibcode:2009A&A...505..205D, doi:10.1051/0004-6361/200911976, S2CID 14786643. See Table B.1
Saumon, D.; et al. (April 1996), "A theory of extrasolar giant planets", The Astrophysical Journal, 460: 993–1018, arXiv:astro-ph/9510046, Bibcode:1996ApJ...460..993S, doi:10.1086/177027, S2CID 18116542.{{citation}}: CS1 maint: numeric names: authors list (link) See Table A1, p. 21.
Kovtyukh, V. V.; et al. (December 2003), "High precision effective temperatures for 181 F-K dwarfs from line-depth ratios", Astronomy and Astrophysics, 411 (3): 559–564, arXiv:astro-ph/0308429, Bibcode:2003A&A...411..559K, doi:10.1051/0004-6361:20031378, S2CID 18478960.
Santos, N. C.; Israelian, G.; Mayor, M. (March 2004), "Spectroscopic [Fe/H] for 98 extra-solar planet-host stars: Exploring the probability of planet formation", Astronomy and Astrophysics, 415 (3): 1153–1166, arXiv:astro-ph/0311541, Bibcode:2004A&A...415.1153S, doi:10.1051/0004-6361:20034469, S2CID 11800380.—the percentage of iron is given by ${\begin{smallmatrix}10^{-0.13}=0.74\end{smallmatrix}}$ , or 74%
Roettenbacher, Rachael M.; Cabot, Samuel H. C.; Fischer, Debra A.; Monnier, John D.; Henry, Gregory W.; Harmon, Robert O.; Korhonen, Heidi; Brewer, John M.; Llama, Joe; Petersburg, Ryan R.; Zhao, Lily L.; Kraus, Stefan; Le Bouquin, Jean-Baptiste; Anugu, Narsireddy; Davies, Claire L.; Gardner, Tyler; Lanthermann, Cyprien; Schaefer, Gail; Setterholm, Benjamin; Clark, Catherine A.; Jorstad, Svetlana G.; Kuehn, Kyler; Levine, Stephen (January 2022), "EXPRES. III. Revealing the Stellar Activity Radial Velocity Signature of ϵ Eridani with Photometry and Interferometry", The Astronomical Journal, 163 (1): 19, arXiv:2110.10643, Bibcode:2022AJ....163...19R, doi:10.3847/1538-3881/ac3235, S2CID 239049996.
Fröhlich, H.-E. (December 2007), "The differential rotation of Epsilon Eri from MOST data", Astronomische Nachrichten, 328 (10): 1037–1039, arXiv:0711.0806, Bibcode:2007AN....328.1037F, doi:10.1002/asna.200710876, S2CID 11263751.
Janson, Markus; et al. (February 2015), "High-contrast imaging with Spitzer: deep observations of Vega, Fomalhaut, and ε Eridani", Astronomy & Astrophysics, 574: 10, arXiv:1412.4816, Bibcode:2015A&A...574A.120J, doi:10.1051/0004-6361/201424944, S2CID 118656652, A120.
Janson, M.; et al. (September 2008), "A comprehensive examination of the ε Eridani system. Verification of a 4 micron narrow-band high-contrast imaging approach for planet searches", Astronomy and Astrophysics, 488 (2): 771–780, arXiv:0807.0301, Bibcode:2008A&A...488..771J, doi:10.1051/0004-6361:200809984, S2CID 119113471.
Hatzes, Artie P.; et al. (December 2000), "Evidence for a long-period planet orbiting ε Eridani", The Astrophysical Journal, 544 (2): L145–L148, arXiv:astro-ph/0009423, Bibcode:2000ApJ...544L.145H, doi:10.1086/317319, S2CID 117865372.
Su, Kate Y. L.; et al. (2017), "The Inner 25 au Debris Distribution in the ϵ Eri System", The Astronomical Journal, 153 (5): 226, arXiv:1703.10330, Bibcode:2017AJ....153..226S, doi:10.3847/1538-3881/aa696b, We found that the 24 and 35 μm emission is consistent with the in situ dust distribution produced either by one planetesimal belt at 3–21 au (e.g., Greaves et al. 2014) or by two planetesimal belts at 1.5–2 au (or 3–4 au) and 8–20 au (e.g., a slightly modified form of the proposal in Backman et al. 2009) ... Any planetesimal belt in the inner region of the epsilon Eri system must be located inside 2 au and/or outside 5 au to be dynamically stable with the assumed epsilon Eri b.
Booth, Mark; Pearce, Tim D; Krivov, Alexander V; Wyatt, Mark C; Dent, William R F; Hales, Antonio S; Lestrade, Jean-François; Cruz-Sáenz de Miera, Fernando; Faramaz, Virginie C; Löhne, Torsten; Chavez-Dagostino, Miguel (March 30, 2023). "The clumpy structure of ϵ Eridani's debris disc revisited by ALMA". Monthly Notices of the Royal Astronomical Society. 521 (4). Oxford University Press (OUP): 6180–6194. arXiv:2303.13584. Bibcode:2023MNRAS.521.6180B. doi:10.1093/mnras/stad938. ISSN 0035-8711.
Verbunt, F.; van Gent, R. H. (2012), "The star catalogues of Ptolemaios and Ulugh Beg. Machine-readable versions and comparison with the modern Hipparcos Catalogue", Astronomy & Astrophysics, 544: A31, arXiv:1206.0628, Bibcode:2012A&A...544A..31V, doi:10.1051/0004-6361/201219596, S2CID 54017245.
Verbunt, F.; van Gent, R. H. (2010), "Three editions of the star catalogue of Tycho Brahe. Machine-readable versions and comparison with the modern Hipparcos Catalogue", Astronomy & Astrophysics, 516: A28, arXiv:1003.3836, Bibcode:2010A&A...516A..28V, doi:10.1051/0004-6361/201014002, S2CID 54025412.
Verbunt, F.; van Gent, R. H. (2010), "The star catalogue of Hevelius. Machine-readable version and comparison with the modern Hipparcos Catalogue", Astronomy & Astrophysics, 516: A29, arXiv:1003.3841, Bibcode:2010A&A...516A..29V, doi:10.1051/0004-6361/201014003.
Greaves, J. S.; et al. (October 1998), "A dust ring around Epsilon Eridani: analog to the young Solar System", The Astrophysical Journal, 506 (2): L133–L137, arXiv:astro-ph/9808224, Bibcode:1998ApJ...506L.133G, doi:10.1086/311652, S2CID 15114295.
Janson, Markus; et al. (June 2007), "NACO-SDI Direct Imaging Search for the Exoplanet ε Eri b", The Astronomical Journal, 133 (6): 2442–2456, arXiv:astro-ph/0703300, Bibcode:2007AJ....133.2442J, doi:10.1086/516632, S2CID 56043012.
Vieytes, Mariela C.; Mauas, Pablo J. D.; Díaz, Rodrigo F. (September 2009), "Chromospheric changes in K stars with activity", Monthly Notices of the Royal Astronomical Society, 398 (3): 1495–1504, arXiv:0906.1760, Bibcode:2009MNRAS.398.1495V, doi:10.1111/j.1365-2966.2009.15207.x, S2CID 17768058.
Metcalfe, T. S.; et al. (2016), "Magnetic Activity Cycles in the Exoplanet Host Star epsilon Eridani", The Astrophysical Journal Letters, 763 (2): 6, arXiv:1604.06701, Bibcode:2013ApJ...763L..26M, doi:10.1088/2041-8205/763/2/L26, S2CID 119163275, L26.
Rocha-Pinto, H. J.; et al. (June 2000), "Chemical enrichment and star formation in the Milky Way disk. I. Sample description and chromospheric age-metallicity relation", Astronomy and Astrophysics, 358: 850–868, arXiv:astro-ph/0001382, Bibcode:2000A&A...358..850R.
Gai, Ning; Bi, Shao-Lan; Tang, Yan-Ke (October 2008), "Modeling ε Eri and asteroseismic tests of element diffusion", Chinese Journal of Astronomy and Astrophysics, 8 (5): 591–602, arXiv:0806.1811, Bibcode:2008ChJAA...8..591G, doi:10.1088/1009-9271/8/5/10, S2CID 16642862.
Ness, J.-U.; Jordan, C. (April 2008), "The corona and upper transition region of ε Eridani", Monthly Notices of the Royal Astronomical Society, 385 (4): 1691–1708, arXiv:0711.3805, Bibcode:2008MNRAS.385.1691N, doi:10.1111/j.1365-2966.2007.12757.x, S2CID 17396544.
Coffaro, M.; et al. (April 2020), "An X-ray activity cycle on the young solar-like star ɛ Eridani", Astronomy & Astrophysics, 636: 18, arXiv:2002.11009, Bibcode:2020A&A...636A..49C, doi:10.1051/0004-6361/201936479, S2CID 211296501, A49.
Wood, Brian E.; Müller, Hans-Reinhard; Zank, Gary P.; Linsky, Jeffrey L. (July 2002), "Measured mass-loss rates of solar-like stars as a function of age and activity", The Astrophysical Journal, 574 (1): 412–425, arXiv:astro-ph/0203437, Bibcode:2002ApJ...574..412W, doi:10.1086/340797, S2CID 1500425. See p. 10.
de Mello, G. F. Porto; del Peloso, E. F.; Ghezzi, Luan (2006), "Astrobiologically interesting stars within 10 parsecs of the Sun", Astrobiology, 6 (2): 308–331, arXiv:astro-ph/0511180, Bibcode:2006AsBio...6..308P, doi:10.1089/ast.2006.6.308, PMID 16689649, S2CID 119459291.
Deltorn, J.-M.; Greene, P. (May 16, 2001), "Search for nemesis encounters with Vega, epsilon Eridani, and Fomalhaut", in Jayawardhana, Ray; Greene, Thoas (eds.), Young Stars Near Earth: Progress and Prospects, Astronomical Society of the Pacific Conference Series, vol. 244, San Francisco, CA: Astronomical Society of the Pacific, pp. 227–232, arXiv:astro-ph/0105284, Bibcode:2001ASPC..244..227D, ISBN 1-58381-082-X.
Potemine, Igor Yu. (April 12, 2010). "Transit of Luyten 726-8 within 1 ly from Epsilon Eridani". arXiv:1004.1557 [astro-ph.SR].
Backman, D.; et al. (2009), "Epsilon Eridani's planetary debris disk: structure and dynamics based on Spitzer and CSO observations", The Astrophysical Journal, 690 (2): 1522–1538, arXiv:0810.4564, Bibcode:2009ApJ...690.1522B, doi:10.1088/0004-637X/690/2/1522, S2CID 18183427.
Feng, Fabo; Butler, R. Paul; et al. (July 2023). "Revised orbits of the two nearest Jupiters". Monthly Notices of the Royal Astronomical Society. 525: 607–619. arXiv:2307.13622. Bibcode:2023MNRAS.525..607F. doi:10.1093/mnras/stad2297.
Reidemeister, M.; et al. (March 2011), "The cold origin of the warm dust around ε Eridani", Astronomy & Astrophysics, 527: A57, arXiv:1011.4882, Bibcode:2011A&A...527A..57R, doi:10.1051/0004-6361/201015328, S2CID 56019152.
Davis, G. R.; et al. (February 2005), "Structure in the ε Eridani debris disk", The Astrophysical Journal, 619 (2): L187–L190, arXiv:astro-ph/0208279, Bibcode:2005ApJ...619L.187G, doi:10.1086/428348, S2CID 121935302.
Ozernoy, Leonid M.; Gorkavyi, Nick N.; Mather, John C.; Taidakova, Tanya A. (July 2000), "Signatures of exosolar planets in dust debris disks", The Astrophysical Journal Letters, 537 (2): L147–L151, arXiv:astro-ph/0007014, Bibcode:2000ApJ...537L.147O, doi:10.1086/312779, S2CID 1149097.
Quillen, A. C.; Thorndike, Stephen (October 2002), "Structure in the ε Eridani dusty disk caused by mean motion resonances with a 0.3 eccentricity planet at periastron", The Astrophysical Journal, 578 (2): L149–L142, arXiv:astro-ph/0208279, Bibcode:2002ApJ...578L.149Q, doi:10.1086/344708, S2CID 955461.
Deller, A. T.; Maddison, S. T. (May 20, 2005). "Numerical Modeling of Dusty Debris Disks". The Astrophysical Journal. 625 (1). American Astronomical Society: 398–413. arXiv:astro-ph/0502135. Bibcode:2005ApJ...625..398D. doi:10.1086/429365. ISSN 0004-637X. S2CID 2764643.
Chavez-Dagostino, M.; Bertone, E.; Cruz-Saenz de Miera, F.; Marshall, J. P.; Wilson, G. W.; Sánchez-Argüelles, D.; Hughes, D. H.; Kennedy, G.; Vega, O.; De la Luz, V.; Dent, W. R. F.; Eiroa, C.; Gómez-Ruiz, A. I.; Greaves, J. S.; Lizano, S.; López-Valdivia, R.; Mamajek, E.; Montaña, A.; Olmedo, M.; Rodríguez-Montoya, I.; Schloerb, F. P.; Yun, Min S.; Zavala, J. A.; Zeballos, M. (June 8, 2016). "Early science with the Large Millimetre Telescope: Deep LMT/AzTEC millimetre observations of ϵ Eridani and its surroundings". Monthly Notices of the Royal Astronomical Society. 462 (3). Oxford University Press (OUP): 2285–2294. arXiv:1606.02761. doi:10.1093/mnras/stw1363. ISSN 0035-8711.
Setiawan, J.; et al. (2008), "Planets Around Active Stars", in Santos, N.C.; Pasquini, L.; Correia, A.; Romaniello, M (eds.), Precision Spectroscopy in Astrophysics, ESO Astrophysics Symposia, Garching, Germany: European Southern Observatory, pp. 201–204, arXiv:0704.2145, Bibcode:2008psa..conf..201S, doi:10.1007/978-3-540-75485-5_43, ISBN 978-3-540-75484-8, S2CID 116889047.
Heinze, A. N.; et al. (November 2008), "Deep L'- and M-band imaging for planets around Vega and ε Eridani", The Astrophysical Journal, 688 (1): 583–596, arXiv:0807.3975, Bibcode:2008ApJ...688..583H, doi:10.1086/592100, S2CID 17082115.
Zechmeister, M.; et al. (April 2013), "The planet search programme at the ESO Coudé Echelle spectrometer and HARPS. IV. The search for Jupiter analogues around solar-like stars", Astronomy & Astrophysics, 552: 62, arXiv:1211.7263, Bibcode:2013A&A...552A..78Z, doi:10.1051/0004-6361/201116551, S2CID 53694238, A78.
Mawet, Dimitri; Hirsch, Lea; et al. (2019), "Deep Exploration of ϵ Eridani with Keck Ms-band Vortex Coronagraphy and Radial Velocities: Mass and Orbital Parameters of the Giant Exoplanet" (PDF), The Astronomical Journal, 157 (1): 33, arXiv:1810.03794, Bibcode:2019AJ....157...33M, doi:10.3847/1538-3881/aaef8a, ISSN 1538-3881, OCLC 7964711337, S2CID 119350738, In this paper, we have presented the most sensitive and comprehensive observational evidence for the existence of ε Eridani b.
Makarov, Valeri V.; Zacharias, Norbert; Finch, Charles T. (2021), "Looking for Astrometric Signals below 20 m s−1: A Jupiter-mass Planet Signature in ε Eri", Research Notes of the AAS, 5 (6): 155, arXiv:2107.01090, Bibcode:2021RNAAS...5..155M, doi:10.3847/2515-5172/ac0f59, We conclude that the newest astrometric results confirm the existence of a long-period exoplanet orbiting ε Eri....The results are consistent with the previously reported planet epsEri-b of approximately Jupiter mass and a period of several years.
Llop-Sayson, Jorge; Wang, Jason J.; et al. (November 2021). "Constraining the Orbit and Mass of epsilon Eridani b with Radial Velocities, Hipparcos IAD-Gaia DR2 Astrometry, and Multiepoch Vortex Coronagraphy Upper Limits". The Astronomical Journal. 162 (5): 181. arXiv:2108.02305. Bibcode:2021AJ....162..181L. doi:10.3847/1538-3881/ac134a. 181.
Butler, R. P.; et al. (2006), "Catalog of nearby exoplanets", The Astrophysical Journal, 646 (1): 505–522, arXiv:astro-ph/0607493, Bibcode:2006ApJ...646..505B, doi:10.1086/504701, S2CID 119067572.
Kitzmann, D.; et al. (February 2010), "Clouds in the atmospheres of extrasolar planets. I. Climatic effects of multi-layered clouds for Earth-like planets and implications for habitable zones", Astronomy and Astrophysics, 511: 511A66.1–511A66.14, arXiv:1002.2927, Bibcode:2010A&A...511A..66K, doi:10.1051/0004-6361/200913491, S2CID 56345031. See table 3.
Underwood, David R.; Jones, Barrie W.; Sleep, P. Nick (2003), "The evolution of habitable zones during stellar lifetimes and its implications on the search for extraterrestrial life", International Journal of Astrobiology, 2 (4): 289–299, arXiv:astro-ph/0312522, Bibcode:2003IJAsB...2..289U, doi:10.1017/S1473550404001715, S2CID 119496186.
Jones, Barrie W.; Underwood, David R.; Sleep, P. Nick (April 22–25, 2003), "The stability of the orbits of Earth-mass planets in and near the habitable zones of known exoplanetary systems", Proceedings of the Conference on Towards Other Earths: DARWIN/TPF and the Search for Extrasolar Terrestrial Planets, 539, Heidelberg, Germany: Dordrecht, D. Reidel Publishing Co: 625–630, arXiv:astro-ph/0305500, Bibcode:2003ESASP.539..625J, ISBN 92-9092-849-2.
Buccino, A. P.; Lemarchand, G. A.; Mauas, P. J. D. (2006), "Ultraviolet radiation constraints around the circumstellar habitable zones", Icarus, 183 (2): 491–503, arXiv:astro-ph/0512291, Bibcode:2006Icar..183..491B, doi:10.1016/j.icarus.2006.03.007, ISSN 0019-1035, S2CID 2241081, In near the 41% stars of the sample: HD19994, 70 Vir, 14 Her, 55 Cnc, 47 UMa, ε Eri and HD3651, there is no coincidence at all between the UV region and the HZ...the traditional HZ would not be habitable following the UV criteria exposed in this work.

astromyth.ru

Звёздный каталог ал-Бируни с приложением каталогов Хайяма и ат-Туси. djvu Archived March 4, 2016, at the Wayback Machine. (Epsilon Eridani: see page 135).

bbc.co.uk

news.bbc.co.uk

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books.google.com

From Epsilon Eridani, the Sun would appear on the diametrically opposite side of the sky at the coordinates RA=15^h 32^m 55.84496^s, Dec=+09° 27′ 29.7312″, which is located near Alpha Serpentis. The absolute magnitude of the Sun is 4.83,^[a] so, at a distance of 3.212 parsecs, the Sun would have an apparent magnitude: ${\begin{smallmatrix}m=M_{v}+5\cdot \log _{10}(3.212/10)+A_{V}=2.36\end{smallmatrix}}$ ${\begin{smallmatrix}m=M_{v}+5\cdot \log _{10}(3.212/10)+A_{V}=2.36\end{smallmatrix}}$ ,^[b] assuming negligible extinction (A_V) for a nearby star.
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3. Lacaille, Nicolas Louis de. (1755). "Ephemerides des mouvemens celestes, pour dix années, depuis 1755 jusqu'en 1765, et pour le meridien de la ville de Paris". Paris. Google Books id: CGHtdxdcc5UC. (Epsilon Eridani: see page LV of the "Introduction").
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Mawet, Dimitri; Hirsch, Lea; et al. (2019), "Deep Exploration of ϵ Eridani with Keck Ms-band Vortex Coronagraphy and Radial Velocities: Mass and Orbital Parameters of the Giant Exoplanet" (PDF), The Astronomical Journal, 157 (1): 33, arXiv:1810.03794, Bibcode:2019AJ....157...33M, doi:10.3847/1538-3881/aaef8a, ISSN 1538-3881, OCLC 7964711337, S2CID 119350738, In this paper, we have presented the most sensitive and comprehensive observational evidence for the existence of ε Eridani b.
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