Харвардска спектрална класификација (Serbian Wikipedia)

Analysis of information sources in references of the Wikipedia article "Харвардска спектрална класификација" in Serbian language version.

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5harvard.edu

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3semanticscholar.org

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3arxiv.org

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2csiro.au

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1vendian.org

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1psu.edu

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archive.org

Moore, Patrick (1992). The Guinness Book of Astronomy: Facts & Feats (4th изд.). Guinness. ISBN 978-0-85112-940-2.
Ledrew, Glenn (фебруар 2001). „The Real Starry Sky”. Journal of the Royal Astronomical Society of Canada. 95: 32. Bibcode:2001JRASC..95...32L.

arxiv.org

Weidner, Carsten; Vink, Jorick S. (децембар 2010). „The masses, and the mass discrepancy of O-type stars”. Astronomy and Astrophysics. 524. A98. Bibcode:2010A&A...524A..98W. S2CID 118836634. arXiv:1010.2204 . doi:10.1051/0004-6361/201014491.
Baraffe, I.; Chabrier, G.; Barman, T. S.; Allard, F.; Hauschildt, P. H. (мај 2003). „Evolutionary models for cool brown dwarfs and extrasolar giant planets. The case of HD 209458”. Astronomy and Astrophysics. 402 (2): 701—712. Bibcode:2003A&A...402..701B. S2CID 15838318. arXiv:astro-ph/0302293 . doi:10.1051/0004-6361:20030252.
Sota, A.; Maíz Apellániz, J.; Morrell, N. I.; Barbá, R. H.; Walborn, N. R.; et al. (март 2014). „The Galactic O-Star Spectroscopic Survey (GOSSS). II. Bright Southern Stars”. The Astrophysical Journal Supplement Series. 211 (1). 10. Bibcode:2014ApJS..211...10S. S2CID 118847528. arXiv:1312.6222 . doi:10.1088/0067-0049/211/1/10.

csiro.au

atnf.csiro.au

„The Colour of Stars”. Australia Telescope National Facility. 2018-10-17.

outreach.atnf.csiro.au

„The Colour of Stars”. Australia Telescope Outreach and Education. 21. 12. 2004. Архивирано из оригинала 10. 03. 2012. г. Приступљено 26. 9. 2007. — Explains the reason for the difference in color perception.

doi.org

Weidner, Carsten; Vink, Jorick S. (децембар 2010). „The masses, and the mass discrepancy of O-type stars”. Astronomy and Astrophysics. 524. A98. Bibcode:2010A&A...524A..98W. S2CID 118836634. arXiv:1010.2204 . doi:10.1051/0004-6361/201014491.
Baraffe, I.; Chabrier, G.; Barman, T. S.; Allard, F.; Hauschildt, P. H. (мај 2003). „Evolutionary models for cool brown dwarfs and extrasolar giant planets. The case of HD 209458”. Astronomy and Astrophysics. 402 (2): 701—712. Bibcode:2003A&A...402..701B. S2CID 15838318. arXiv:astro-ph/0302293 . doi:10.1051/0004-6361:20030252.
Sota, A.; Maíz Apellániz, J.; Morrell, N. I.; Barbá, R. H.; Walborn, N. R.; et al. (март 2014). „The Galactic O-Star Spectroscopic Survey (GOSSS). II. Bright Southern Stars”. The Astrophysical Journal Supplement Series. 211 (1). 10. Bibcode:2014ApJS..211...10S. S2CID 118847528. arXiv:1312.6222 . doi:10.1088/0067-0049/211/1/10.

harvard.edu

adsabs.harvard.edu

Habets, G. M. H. J.; Heinze, J. R. W. (новембар 1981). „Empirical bolometric corrections for the main-sequence”. Astronomy and Astrophysics Supplement Series. 46: 193—237 (Tables VII and VIII). Bibcode:1981A&AS...46..193H. – Luminosities are derived from M_bol figures, using M_bol(☉)=4.75.
Weidner, Carsten; Vink, Jorick S. (децембар 2010). „The masses, and the mass discrepancy of O-type stars”. Astronomy and Astrophysics. 524. A98. Bibcode:2010A&A...524A..98W. S2CID 118836634. arXiv:1010.2204 . doi:10.1051/0004-6361/201014491.
Baraffe, I.; Chabrier, G.; Barman, T. S.; Allard, F.; Hauschildt, P. H. (мај 2003). „Evolutionary models for cool brown dwarfs and extrasolar giant planets. The case of HD 209458”. Astronomy and Astrophysics. 402 (2): 701—712. Bibcode:2003A&A...402..701B. S2CID 15838318. arXiv:astro-ph/0302293 . doi:10.1051/0004-6361:20030252.
Ledrew, Glenn (фебруар 2001). „The Real Starry Sky”. Journal of the Royal Astronomical Society of Canada. 95: 32. Bibcode:2001JRASC..95...32L.
Sota, A.; Maíz Apellániz, J.; Morrell, N. I.; Barbá, R. H.; Walborn, N. R.; et al. (март 2014). „The Galactic O-Star Spectroscopic Survey (GOSSS). II. Bright Southern Stars”. The Astrophysical Journal Supplement Series. 211 (1). 10. Bibcode:2014ApJS..211...10S. S2CID 118847528. arXiv:1312.6222 . doi:10.1088/0067-0049/211/1/10.

psu.edu

e-education.psu.edu

Palma, Dr. Christopher (2016). „The Hertzsprung-Russell Diagram”. ASTRO 801: Planets, Stars, Galaxies, and the Universe. John A. Dutton e-Education Institute: College of Earth and Mineral Sciences: The Pennsylvania State University. Приступљено 2017-01-29. „The quantities that are easiest to measure... are color and magnitude, so most observers ... refer to the diagram as a 'Color–Magnitude diagram' or 'CMD' rather than an HR diagram.”

semanticscholar.org

api.semanticscholar.org

Weidner, Carsten; Vink, Jorick S. (децембар 2010). „The masses, and the mass discrepancy of O-type stars”. Astronomy and Astrophysics. 524. A98. Bibcode:2010A&A...524A..98W. S2CID 118836634. arXiv:1010.2204 . doi:10.1051/0004-6361/201014491.
Baraffe, I.; Chabrier, G.; Barman, T. S.; Allard, F.; Hauschildt, P. H. (мај 2003). „Evolutionary models for cool brown dwarfs and extrasolar giant planets. The case of HD 209458”. Astronomy and Astrophysics. 402 (2): 701—712. Bibcode:2003A&A...402..701B. S2CID 15838318. arXiv:astro-ph/0302293 . doi:10.1051/0004-6361:20030252.
Sota, A.; Maíz Apellániz, J.; Morrell, N. I.; Barbá, R. H.; Walborn, N. R.; et al. (март 2014). „The Galactic O-Star Spectroscopic Survey (GOSSS). II. Bright Southern Stars”. The Astrophysical Journal Supplement Series. 211 (1). 10. Bibcode:2014ApJS..211...10S. S2CID 118847528. arXiv:1312.6222 . doi:10.1088/0067-0049/211/1/10.

vendian.org

Charity, Mitchell. „What color are the stars?”. Vendian.org. Приступљено 13. 5. 2006.

webcitation.org

„The Colour of Stars”. Australia Telescope Outreach and Education. 21. 12. 2004. Архивирано из оригинала 10. 03. 2012. г. Приступљено 26. 9. 2007. — Explains the reason for the difference in color perception.