Bolometric correction (English Wikipedia)

Analysis of information sources in references of the Wikipedia article "Bolometric correction" in English language version.

refsWebsite

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9harvard.edu

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8doi.org

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6arxiv.org

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4worldcat.org

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3semanticscholar.org

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1github.com

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1iau.org

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1iop.org

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arxiv.org

Salaris, Maurizio; et al. (November 2002). "Population effects on the red giant clump absolute magnitude: the K band". Monthly Notices of the Royal Astronomical Society. 337 (1): 332–340. arXiv:astro-ph/0208057. Bibcode:2002MNRAS.337..332S. doi:10.1046/j.1365-8711.2002.05917.x. S2CID 17930469. Lower effective temperatures correspond to higher values of $BC_{K}$ ; since $M_{K}=M_{bol}-BC_{K}\!\,$ , cooler RC stars tend to be brighter.
Buzzoni, A.; et al. (April 2010). "Bolometric correction and spectral energy distribution of cool stars in Galactic clusters". Monthly Notices of the Royal Astronomical Society. 403 (3): 1592–1610. arXiv:1002.1972. Bibcode:2010MNRAS.403.1592B. doi:10.1111/j.1365-2966.2009.16223.x. S2CID 119181086.
Casagrande, Luca; VandenBerg, Don A. (October 2014), "Synthetic stellar photometry: general considerations and new transformations for broad-band systems", Monthly Notices of the Royal Astronomical Society, 444 (1): 392, arXiv:1407.6095, Bibcode:2014MNRAS.444..392C, doi:10.1093/mnras/stu1476 with up-to-date interpolation codes https://github.com/casaluca/bolometric-corrections
Casagrande, L; VandenBerg, Don A (2018-01-18). "Synthetic Stellar Photometry – II. Testing the bolometric flux scale and tables of bolometric corrections for the Hipparcos/Tycho, Pan-STARRS1, SkyMapper, and JWST systems". Monthly Notices of the Royal Astronomical Society. 475 (4): 5023–5040. arXiv:1801.05508. Bibcode:2018MNRAS.475.5023C. doi:10.1093/mnras/sty149. ISSN 0035-8711.
Mamajek, E. E.; et al. (2015). "IAU 2015 Resolution B2 on Recommended Zero Points for the Absolute and Apparent Bolometric Magnitude Scales". arXiv:1510.06262v2 [astro-ph.SR].
Torres, Guillermo (November 2010). "On the Use of Empirical Bolometric Corrections for Stars". The Astronomical Journal. 140 (5): 1158–1162. arXiv:1008.3913. Bibcode:2010AJ....140.1158T. doi:10.1088/0004-6256/140/5/1158. S2CID 119219274.

doi.org

Popper, Daniel M. (1980-09-01). "Stellar Masses". Annual Review of Astronomy and Astrophysics. 18 (1): 115–164. Bibcode:1980ARA&A..18..115P. doi:10.1146/annurev.aa.18.090180.000555. ISSN 0066-4146.
Humphreys, R. M.; McElroy, D. B. (1984). "The initial mass function for massive stars in the Galaxy and the Magellanic Clouds". The Astrophysical Journal. 284: 565–577. Bibcode:1984ApJ...284..565H. doi:10.1086/162439. ISSN 0004-637X.
Salaris, Maurizio; et al. (November 2002). "Population effects on the red giant clump absolute magnitude: the K band". Monthly Notices of the Royal Astronomical Society. 337 (1): 332–340. arXiv:astro-ph/0208057. Bibcode:2002MNRAS.337..332S. doi:10.1046/j.1365-8711.2002.05917.x. S2CID 17930469. Lower effective temperatures correspond to higher values of $BC_{K}$ ; since $M_{K}=M_{bol}-BC_{K}\!\,$ , cooler RC stars tend to be brighter.
Buzzoni, A.; et al. (April 2010). "Bolometric correction and spectral energy distribution of cool stars in Galactic clusters". Monthly Notices of the Royal Astronomical Society. 403 (3): 1592–1610. arXiv:1002.1972. Bibcode:2010MNRAS.403.1592B. doi:10.1111/j.1365-2966.2009.16223.x. S2CID 119181086.
Casagrande, Luca; VandenBerg, Don A. (October 2014), "Synthetic stellar photometry: general considerations and new transformations for broad-band systems", Monthly Notices of the Royal Astronomical Society, 444 (1): 392, arXiv:1407.6095, Bibcode:2014MNRAS.444..392C, doi:10.1093/mnras/stu1476 with up-to-date interpolation codes https://github.com/casaluca/bolometric-corrections
Casagrande, L; VandenBerg, Don A (2018-01-18). "Synthetic Stellar Photometry – II. Testing the bolometric flux scale and tables of bolometric corrections for the Hipparcos/Tycho, Pan-STARRS1, SkyMapper, and JWST systems". Monthly Notices of the Royal Astronomical Society. 475 (4): 5023–5040. arXiv:1801.05508. Bibcode:2018MNRAS.475.5023C. doi:10.1093/mnras/sty149. ISSN 0035-8711.
Flower, Phillip J. (September 1996), "Transformations from Theoretical Hertzsprung-Russell Diagrams to Color-Magnitude Diagrams: Effective Temperatures, B-V Colors, and Bolometric Corrections", The Astrophysical Journal, 469: 355, Bibcode:1996ApJ...469..355F, doi:10.1086/177785
Torres, Guillermo (November 2010). "On the Use of Empirical Bolometric Corrections for Stars". The Astronomical Journal. 140 (5): 1158–1162. arXiv:1008.3913. Bibcode:2010AJ....140.1158T. doi:10.1088/0004-6256/140/5/1158. S2CID 119219274.

github.com

Casagrande, Luca; VandenBerg, Don A. (October 2014), "Synthetic stellar photometry: general considerations and new transformations for broad-band systems", Monthly Notices of the Royal Astronomical Society, 444 (1): 392, arXiv:1407.6095, Bibcode:2014MNRAS.444..392C, doi:10.1093/mnras/stu1476 with up-to-date interpolation codes https://github.com/casaluca/bolometric-corrections

harvard.edu

ui.adsabs.harvard.edu

Popper, Daniel M. (1980-09-01). "Stellar Masses". Annual Review of Astronomy and Astrophysics. 18 (1): 115–164. Bibcode:1980ARA&A..18..115P. doi:10.1146/annurev.aa.18.090180.000555. ISSN 0066-4146.
Humphreys, R. M.; McElroy, D. B. (1984). "The initial mass function for massive stars in the Galaxy and the Magellanic Clouds". The Astrophysical Journal. 284: 565–577. Bibcode:1984ApJ...284..565H. doi:10.1086/162439. ISSN 0004-637X.
Bessell, M. S.; et al. (May 1998). "Model atmospheres broad-band colors, bolometric corrections and temperature calibrations for O - M stars". Astronomy and Astrophysics. 333: 231–250. Bibcode:1998A&A...333..231B.
Salaris, Maurizio; et al. (November 2002). "Population effects on the red giant clump absolute magnitude: the K band". Monthly Notices of the Royal Astronomical Society. 337 (1): 332–340. arXiv:astro-ph/0208057. Bibcode:2002MNRAS.337..332S. doi:10.1046/j.1365-8711.2002.05917.x. S2CID 17930469. Lower effective temperatures correspond to higher values of $BC_{K}$ ; since $M_{K}=M_{bol}-BC_{K}\!\,$ , cooler RC stars tend to be brighter.
Buzzoni, A.; et al. (April 2010). "Bolometric correction and spectral energy distribution of cool stars in Galactic clusters". Monthly Notices of the Royal Astronomical Society. 403 (3): 1592–1610. arXiv:1002.1972. Bibcode:2010MNRAS.403.1592B. doi:10.1111/j.1365-2966.2009.16223.x. S2CID 119181086.
Casagrande, Luca; VandenBerg, Don A. (October 2014), "Synthetic stellar photometry: general considerations and new transformations for broad-band systems", Monthly Notices of the Royal Astronomical Society, 444 (1): 392, arXiv:1407.6095, Bibcode:2014MNRAS.444..392C, doi:10.1093/mnras/stu1476 with up-to-date interpolation codes https://github.com/casaluca/bolometric-corrections
Casagrande, L; VandenBerg, Don A (2018-01-18). "Synthetic Stellar Photometry – II. Testing the bolometric flux scale and tables of bolometric corrections for the Hipparcos/Tycho, Pan-STARRS1, SkyMapper, and JWST systems". Monthly Notices of the Royal Astronomical Society. 475 (4): 5023–5040. arXiv:1801.05508. Bibcode:2018MNRAS.475.5023C. doi:10.1093/mnras/sty149. ISSN 0035-8711.
Flower, Phillip J. (September 1996), "Transformations from Theoretical Hertzsprung-Russell Diagrams to Color-Magnitude Diagrams: Effective Temperatures, B-V Colors, and Bolometric Corrections", The Astrophysical Journal, 469: 355, Bibcode:1996ApJ...469..355F, doi:10.1086/177785
Torres, Guillermo (November 2010). "On the Use of Empirical Bolometric Corrections for Stars". The Astronomical Journal. 140 (5): 1158–1162. arXiv:1008.3913. Bibcode:2010AJ....140.1158T. doi:10.1088/0004-6256/140/5/1158. S2CID 119219274.

iau.org

IAU XXIX General Assembly Draft Resolutions Announced, retrieved 2015-07-08

iop.org

iopscience.iop.org

Torres, Guillermo (November 2010). "On the Use of Empirical Bolometric Corrections for Stars". The Astronomical Journal. 140 (5): 1158–1162. arXiv:1008.3913. Bibcode:2010AJ....140.1158T. doi:10.1088/0004-6256/140/5/1158. S2CID 119219274.

semanticscholar.org

api.semanticscholar.org

Salaris, Maurizio; et al. (November 2002). "Population effects on the red giant clump absolute magnitude: the K band". Monthly Notices of the Royal Astronomical Society. 337 (1): 332–340. arXiv:astro-ph/0208057. Bibcode:2002MNRAS.337..332S. doi:10.1046/j.1365-8711.2002.05917.x. S2CID 17930469. Lower effective temperatures correspond to higher values of $BC_{K}$ ; since $M_{K}=M_{bol}-BC_{K}\!\,$ , cooler RC stars tend to be brighter.
Buzzoni, A.; et al. (April 2010). "Bolometric correction and spectral energy distribution of cool stars in Galactic clusters". Monthly Notices of the Royal Astronomical Society. 403 (3): 1592–1610. arXiv:1002.1972. Bibcode:2010MNRAS.403.1592B. doi:10.1111/j.1365-2966.2009.16223.x. S2CID 119181086.
Torres, Guillermo (November 2010). "On the Use of Empirical Bolometric Corrections for Stars". The Astronomical Journal. 140 (5): 1158–1162. arXiv:1008.3913. Bibcode:2010AJ....140.1158T. doi:10.1088/0004-6256/140/5/1158. S2CID 119219274.

worldcat.org

search.worldcat.org

Popper, Daniel M. (1980-09-01). "Stellar Masses". Annual Review of Astronomy and Astrophysics. 18 (1): 115–164. Bibcode:1980ARA&A..18..115P. doi:10.1146/annurev.aa.18.090180.000555. ISSN 0066-4146.
Humphreys, R. M.; McElroy, D. B. (1984). "The initial mass function for massive stars in the Galaxy and the Magellanic Clouds". The Astrophysical Journal. 284: 565–577. Bibcode:1984ApJ...284..565H. doi:10.1086/162439. ISSN 0004-637X.
B., Kaler, James (1989). Stars and their spectra: an introduction to the spectral sequence. Cambridge [Cambridgeshire]: Cambridge University Press. ISBN 978-0521304948. OCLC 17731797.{{cite book}}: CS1 maint: multiple names: authors list (link)
Casagrande, L; VandenBerg, Don A (2018-01-18). "Synthetic Stellar Photometry – II. Testing the bolometric flux scale and tables of bolometric corrections for the Hipparcos/Tycho, Pan-STARRS1, SkyMapper, and JWST systems". Monthly Notices of the Royal Astronomical Society. 475 (4): 5023–5040. arXiv:1801.05508. Bibcode:2018MNRAS.475.5023C. doi:10.1093/mnras/sty149. ISSN 0035-8711.