광도 순 항성 목록
같이 보기

↑  Crowther, P. A.; Lennon, D. J.; Walborn, N. R. (January 2006), “Physical parameters and wind properties of galactic early B supergiants”, 《Astronomy and Astrophysics》 446 (1): 279–293, arXiv:astro-ph/0509436, Bibcode:2006A&A...446..279C, doi:10.1051/0004-6361:20053685, S2CID 18815761
↑  Simón-Díaz, S.; Herrero, A.; Esteban, C.; Najarro, F. (2006). “Detailed spectroscopic analysis of the Trapezium cluster stars inside the Orion nebula: Rotational velocities, stellar parameters, and oxygen abundances”. 《Astronomy & Astrophysics》 448 (1): 351–366. arXiv:astro-ph/0510288. Bibcode:2006A&A...448..351S. doi:10.1051/0004-6361:20053066. ISSN 0004-6361. S2CID 16445304.
↑  Shenar, T.; Oskinova, L.; Hamann, W.-R.; Corcoran, M. F.; Moffat, A. F. J.; Pablo, H.; Richardson, N. D.; Waldron, W. L.; Huenemoerder, D. P.; Maíz Apellániz, J.; Nichols, J. S.; Todt, H.; Nazé, Y.; Hoffman, J. L.; Pollock, A. M. T.; Negueruela, I. (2015). “A Coordinated X-Ray and Optical Campaign of the Nearest Massive Eclipsing Binary, δ Orionis Aa. IV. A Multiwavelength, Non-LTE Spectroscopic Analysis”. 《Astrophysical Journal》 809 (2): 135. arXiv:1503.03476. Bibcode:2015ApJ...809..135S. doi:10.1088/0004-637X/809/2/135. hdl:10045/59172. S2CID 14909574.
↑  Tokovinin, A. A. (1997). “MSC - a catalogue of physical multiple stars”. 《Astronomy and Astrophysics Supplement Series》 124: 75–84. Bibcode:1997A&AS..124...75T. doi:10.1051/aas:1997181.
↑  Dufton, P. L.; Smartt, S. J.; Lee, J. K.; Ryans, R. S. I.; Hunter, I.; Evans, C. J.; Herrero, A.; Trundle, C.; Lennon, D. J.; Irwin, M. J.; Kaufer, A. (2006). “The VLT-FLAMES survey of massive stars: stellar parameters and rotational velocities in NGC 3293, NGC 4755 and NGC 6611”. 《Astronomy & Astrophysics》 457 (1): 265–280. arXiv:astro-ph/0606409. Bibcode:2006A&A...457..265D. doi:10.1051/0004-6361:20065392. ISSN 0004-6361. S2CID 15874925.
↑  Murdin, P.; Penston, M. V. (1977년 12월 1일). “The Lambda Orionis association”. 《Monthly Notices of the Royal Astronomical Society》 181 (4): 657–665. Bibcode:1977MNRAS.181..657M. doi:10.1093/mnras/181.4.657. ISSN 0035-8711.
1 2 3  Hoffleit, Dorrit; Jaschek, Carlos (1991). 《The Bright star catalogue》 5 Revis판. New Haven, Conn.: Yale University Observatory. Bibcode:1991bsc..book.....H.
↑  Moravveji, Ehsan; Guinan, Edward F.; Shultz, Matt; Williamson, Michael H.; Moya, Andres (2012년 3월 10일). “Asteroseismology of the Nearby SN-II Progenitor: Rigel. I. Themosthigh-Precision Photometry and Radial Velocity Monitoring”. 《The Astrophysical Journal》 747 (2): 108. arXiv:1201.0843. Bibcode:2012ApJ...747..108M. doi:10.1088/0004-637X/747/2/108. ISSN 0004-637X. S2CID 425831.
↑  Hillenbrand, Lynne A. (1997). “On the Stellar Population and Star-Forming History of the Orion Nebula Cluster”. 《Astronomical Journal》 113: 1733. Bibcode:1997AJ....113.1733H. doi:10.1086/118389.
↑  Aldoretta, E. J.; Caballero-Nieves, S. M.; Gies, D. R.; Nelan, E. P.; Wallace, D. J.; Hartkopf, W. I.; Henry, T. J.; Jao, W.-C.; Maíz Apellániz, J.; Mason, B. D.; Moffat, A. F. J.; Norris, R. P.; Richardson, N. D.; Williams, S. J. (2015). “The Multiplicity of Massive Stars: A High Angular Resolution Survey with the Guidance Sensor”. 《The Astronomical Journal》 149 (1): 26. arXiv:1410.0021. Bibcode:2015AJ....149...26A. doi:10.1088/0004-6256/149/1/26. S2CID 58911264.
↑  Joyce, Meridith; Leung, Shing-Chi; Molnár, László; Ireland, Michael J.; Kobayashi, Chiaki; Nomoto, Ken'ichi (2020년 10월 13일). “Standing on the shoulders of giants: New mass and distance estimates for Betelgeuse through combined evolutionary, asteroseismic, and hydrodynamical simulations with MESA”. 《The Astrophysical Journal》 902 (1): 63. arXiv:2006.09837. Bibcode:2020ApJ...902...63J. doi:10.3847/1538-4357/abb8db. ISSN 1538-4357.
↑  Nicolet, B. (1978년 10월 1일). “Catalogue of homogeneous data in the UBV photoelectric photometric system.”. 《Astronomy and Astrophysics Supplement Series》 34: 1–49. Bibcode:1978A&AS...34....1N. ISSN 0365-0138.
1 2  Marchenko, Sergey V.; Rauw, Gregor; Antokhina, Eleonora A.; Antokhin, Igor I.; Ballereau, Dominique; Chauville, Jacques; Corcoran, Michael F.; Costero, Rafael; Echevarria, Juan; Eversberg, Thomas; Gayley, Ken G.; Koenigsberger, Gloria; Miroshnichenko, Anatoly S.; Moffat, Anthony F. J.; Morrell, Nidia I.; Morrison, Nancy D.; Mulliss, Christopher L.; Pittard, Julian M.; Stevens, Ian R.; Vreux, Jean-Marie; Zorec, Jean (2000). “Coordinated monitoring of the eccentric O-star binary Iota Orionis: Optical spectroscopy and photometry”. 《Monthly Notices of the Royal Astronomical Society》 317 (2): 333. Bibcode:2000MNRAS.317..333M. doi:10.1046/j.1365-8711.2000.03542.x.
1 2 3  Nicolet, B. (1978), “Photoelectric photometric Catalogue of homogeneous measurements in the UBV System”, 《Astronomy and Astrophysics Supplement Series》 34: 1–49, Bibcode:1978A&AS...34....1N
↑  Underhill, A. B.; Divan, L.; Prevot-Burnichon, M.-L.; Doazan, V. (1979). “Effective temperatures, angular diameters, distances and linear radii for 160 O and B stars”. 《Monthly Notices of the Royal Astronomical Society》 189 (3): 601–05. Bibcode:1979MNRAS.189..601U. doi:10.1093/mnras/189.3.601.
↑  Nieva, M.-F. (2013). “Temperature, gravity, and bolometric correction scales for non-supergiant OB stars”. 《Astronomy & Astrophysics》 550: A26. arXiv:1212.0928. Bibcode:2013A&A...550A..26N. doi:10.1051/0004-6361/201219677. ISSN 0004-6361. S2CID 119275940.
↑  Tanrıverdi, Taner (2013). “Elemental abundances of the supergiant stars σ Cygnus and η Leonis”. 《New Astronomy》 25: 50. arXiv:1512.04557. Bibcode:2013NewA...25...50T. doi:10.1016/j.newast.2013.03.013. S2CID 118525375.
↑  Firnstein, M.; Przybilla, N. (2012). “Quantitative spectroscopy of Galactic BA-type supergiants. I. Atmospheric parameters”. 《Astronomy & Astrophysics》 543: A80. arXiv:1207.0308. Bibcode:2012A&A...543A..80F. doi:10.1051/0004-6361/201219034. S2CID 54725386.
↑  Martins, F.; Schaerer, D.; Hillier, D. J.; Meynadier, F.; Heydari-Malayeri, M.; Walborn, N. R. (2005). “O stars with weak winds: the Galactic case”. 《Astronomy & Astrophysics》 441 (2): 735–762. arXiv:astro-ph/0507278. Bibcode:2005A&A...441..735M. doi:10.1051/0004-6361:20052927. ISSN 0004-6361. S2CID 11547293.
1 2 3  Simón-Díaz, S.; Caballero, J. A.; Lorenzo, J.; Maíz Apellániz, J.; Schneider, F. R. N.; Negueruela, I.; Barbá, R. H.; Dorda, R.; Marco, A.; Montes, D.; Pellerin, A.; Sanchez-Bermudez, J.; Sódor, Á.; Sota, A. (2015). “Orbital and Physical Properties of the σ Ori Aa, Ab, B Triple System”. 《The Astrophysical Journal》 799 (2): 169. arXiv:1412.3469. Bibcode:2015ApJ...799..169S. doi:10.1088/0004-637X/799/2/169. S2CID 118500350.
1 2 3  Mason, Brian D.; Wycoff, Gary L.; Hartkopf, William I.; Douglass, Geoffrey G.; Worley, Charles E. (2001). “The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog”. 《The Astronomical Journal》 122 (6): 3466. Bibcode:2001AJ....122.3466M. doi:10.1086/323920.
↑  Pecaut, Mark J.; Mamajek, Eric E.; Bubar, Eric J. (2012년 2월 20일). “A Revised Age for Upper Scorpius and the Star Formation History Among the F-Type Members of the Scorpius–Centaurus Ob Association”. 《The Astrophysical Journal》 746 (2): 154. arXiv:1112.1695. Bibcode:2012ApJ...746..154P. doi:10.1088/0004-637X/746/2/154. ISSN 0004-637X. S2CID 118461108.
↑  Gutierrez-Moreno, Adelina; Moreno, Hugo (1968년 6월 1일). “A Photometric Investigation of the SCORPlO-CENTAURUS Association”. 《The Astrophysical Journal Supplement Series》 15: 459. Bibcode:1968ApJS...15..459G. doi:10.1086/190168. ISSN 0067-0049.
↑  Lutz, T. E.; Lutz, J. H. (June 1977), “Spectral classification and UBV photometry of bright visual double stars”, 《Astronomical Journal》 82: 431–434, Bibcode:1977AJ.....82..431L, doi:10.1086/112066
1 2 3 4  Johnson, H. L.;  외. (1966), “UBVRIJKL photometry of the bright stars”, 《Communications of the Lunar and Planetary Laboratory》 4 (99): 99, Bibcode:1966CoLPL...4...99J
↑  Hubrig, S.;  외. (June 2006), “Discovery of magnetic fields in the βCephei star ξ1 CMa and in several slowly pulsating B stars*”, 《Monthly Notices of the Royal Astronomical Society: Letters》 369 (1): L61–L65, arXiv:astro-ph/0604283, Bibcode:2006MNRAS.369L..61H, doi:10.1111/j.1745-3933.2006.00175.x, S2CID 18201908
↑  Cousins, A. W. J. (1972), “UBV Photometry of Some Very Bright Stars”, 《Monthly Notes of the Astronomical Society of Southern Africa》 31: 69, Bibcode:1972MNSSA..31...69C
↑  Nieva, María-Fernanda; Przybilla, Norbert (2014). “Fundamental properties of nearby single early B-type stars”. 《Astronomy & Astrophysics》 566: A7. arXiv:1412.1418. Bibcode:2014A&A...566A...7N. doi:10.1051/0004-6361/201423373. S2CID 119227033.
↑  Challouf, M.; Nardetto, N.; Mourard, D.; Graczyk, D.; Aroui, H.; Chesneau, O.; Delaa, O.; Pietrzyński, G.; Gieren, W.; Ligi, R.; Meilland, A.; Perraut, K.; Tallon-Bosc, I.; McAlister, H.; Ten Brummelaar, T.; Sturmann, J.; Sturmann, L.; Turner, N.; Farrington, C.; Vargas, N.; Scott, N. (2014). “Improving the surface brightness-color relation for early-type stars using optical interferometry⋆”. 《Astronomy & Astrophysics》 570: A104. arXiv:1409.1351. Bibcode:2014A&A...570A.104C. doi:10.1051/0004-6361/201423772. S2CID 14624307.
↑  Ducati, J. R. (2002). “VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system.”. 《CDS/ADC Collection of Electronic Catalogues》 2237. Bibcode:2002yCat.2237....0D. S2CID 118191108.
↑  Nicolet, B. (October 1978). “Catalogue of homogeneous data in the UBV photoelectric photometric system”. 《Astronomy and Astrophysics Supplement Series》 34: 1–49. Bibcode:1978A&AS...34....1N.
↑  Pillitteri, I.; Fossati, L.; Castro Rodriguez, N.; Oskinova, L.; Wolk, S. J. (2018). “Detection of magnetic field in the B2 star ρ Ophiuchi A with ESO FORS2”. 《Astronomy & Astrophysics》 610: L3. arXiv:1712.00728. Bibcode:2018A&A...610L...3P. doi:10.1051/0004-6361/201732078. ISSN 0004-6361. S2CID 119395824.
1 2 3 4 5 6 7  Anderson, E.; Francis, Ch. (2012). “XHIP: An extended hipparcos compilation”. 《Astronomy Letters》 38 (5): 331. arXiv:1108.4971. Bibcode:2012AstL...38..331A. doi:10.1134/S1063773712050015. S2CID 119257644.  Vizier catalog entry
↑  Kudritzki, R. P.; Reimers, D. (1978). “On the absolute scale of mass-loss in red giants. II. Circumstellar absorption lines in the spectrum of alpha Sco B and mass-loss of alpha Sco A”. 《Astronomy and Astrophysics》 70: 227. Bibcode:1978A&A....70..227K.
↑  Jerzykiewicz, M.; Molenda-Zakowicz, J. (September 2000), “Empirical Luminosities and Radii of Early-Type Stars after Hipparcos”, 《Acta Astronomica》 50: 369–380, Bibcode:2000AcA....50..369J
↑  Harmanec, P. (2000). “Physical Properties and Evolutionary Stage of Be Stars”. 《The be Phenomenon in Early-Type Stars》 214: 13. Bibcode:2000ASPC..214...13H.
↑  Hubrig, S.; Briquet, M.; De Cat, P.; Schöller, M.; Morel, T.; Ilyin, I. (2009). “New magnetic field measurements of β Cephei stars and slowly pulsating B stars”. 《Astronomische Nachrichten》 330 (4): 317–329. arXiv:0902.1314. Bibcode:2009AN....330..317H. doi:10.1002/asna.200811187. S2CID 17497112.
↑  Fernie, J. D. (May 1983), “New UBVRI photometry for 900 supergiants”, 《Astrophysical Journal Supplement Series》 52: 7–22, Bibcode:1983ApJS...52....7F, doi:10.1086/190856.
↑  Feinstein, A.; Marraco, H. G. (November 1979), “The photometric behavior of Be Stars”, 《Astronomical Journal》 84: 1713–1725, Bibcode:1979AJ.....84.1713F, doi:10.1086/112600.
↑  McDonald, I.;  외. (2012), “Fundamental Parameters and Infrared Excesses of Hipparcos Stars”, 《Monthly Notices of the Royal Astronomical Society》 427 (1): 343–57, arXiv:1208.2037, Bibcode:2012MNRAS.427..343M, doi:10.1111/j.1365-2966.2012.21873.x, S2CID 118665352.
↑  Mermilliod, J.-C. (1986), “Compilation of Eggen's UBV data, transformed to UBV (unpublished)”, 《Catalogue of Eggen's UBV Data》 (SIMBAD), Bibcode:1986EgUBV........0M.
↑  North, P. (1998). “Do SI stars undergo any rotational braking?”. 《Astronomy and Astrophysics》 334: 181–87. arXiv:astro-ph/9802286. Bibcode:1998A&A...334..181N.
↑  Fang, M.;  외. (January 2013), “Young stars in ɛ Chamaleontis and their disks: disk evolution in sparse associations”, 《Astronomy & Astrophysics》 549: 17, arXiv:1209.5832, Bibcode:2013A&A...549A..15F, doi:10.1051/0004-6361/201118528, S2CID 118332644, A15.
↑  Zorec, J.; Royer, F. (2012). “Rotational velocities of A-type stars”. 《Astronomy & Astrophysics》 537: A120. arXiv:1201.2052. Bibcode:2012A&A...537A.120Z. doi:10.1051/0004-6361/201117691. S2CID 55586789.  Vizier catalog entry
↑  Corben, P. M.; Stoy, R. H. (1968), “Photoelectric Magnitudes and Colours for Bright Southern Stars”, 《Monthly Notes of the Astronomical Society of Southern Africa》 27: 11, Bibcode:1968MNSSA..27...11C.
↑  Silaj, J.;  외. (November 2014), “The Hα Profiles of Be Shell Stars”, 《The Astrophysical Journal》 795 (1): 12, Bibcode:2014ApJ...795...82S, doi:10.1088/0004-637X/795/1/82, S2CID 120167606, 82.
↑  Prša, Andrej; Harmanec, Petr; Torres, Guillermo; Mamajek, Eric; Asplund, Martin; Capitaine, Nicole; Christensen-Dalsgaard, Jørgen; Depagne, Éric; Haberreiter, Margit; Hekker, Saskia; Hilton, James; Kopp, Greg; Kostov, Veselin; Kurtz, Donald W.; Laskar, Jacques; Mason, Brian D.; Milone, Eugene F.; Montgomery, Michele; Richards, Mercedes; Schmutz, Werner; Schou, Jesper; Stewart, Susan G. (2016). “Nominal Values for Selected Solar and Planetary Quantities: IAU 2015 Resolution B3”. 《The Astronomical Journal》 152 (2): 41. arXiv:1605.09788. Bibcode:2016AJ....152...41P. doi:10.3847/0004-6256/152/2/41. hdl:1885/108637. S2CID 55319250.
↑  Luzum, Brian; Capitaine, Nicole; Fienga, Agnès; Folkner, William; Fukushima, Toshio; Hilton, James; Hohenkerk, Catherine; Krasinsky, George; Petit, Gérard; Pitjeva, Elena; Soffel, Michael (August 2011). “The IAU 2009 system of astronomical constants: the report of the IAU working group on numerical standards for Fundamental Astronomy”. 《Celestial Mechanics and Dynamical Astronomy》 110 (4): 293–304. Bibcode:2011CeMDA.110..293L. doi:10.1007/s10569-011-9352-4. ISSN 0923-2958.
↑  Bessell, M.S.; Castelli, F.; Plez, B. (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.