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Список на најголеми познати ѕвезди

Од Википедија — слободната енциклопедија
Односни величини на планетите во Сончевиот Систем и неколку познати ѕвезди:

Ова е список на најголемите ѕвезди со познати димензии. Големината е изразена во Сончеви полупречници (прибл. 695.700 км).

Точниот редослед на списокот останува непотполн поради големите недоумици при добивањето на параметрите во пресметките, особено сјајноста и делотворната температура. Многу ѕвездени полупречници можат да се изразат само како просек или во голем вредносен опсег. Вредностите знајачно се разликуваат од еден извор до друг, зависно од брановата должина на набљудување.

Полупречниците на неколку ѕвезди се добиени непосредно по интерферометриски пат. Други се откриени по прикривања (окултации) или од затемнувачки двојки, кои ги испробуваат другите непосредни начини за да ја утврдат вистинската големина. Само неколку корисни суперџиновски ѕвезди подлежат на затскривања од Месечината, какви што се Антарес и Алдебаран. Примери за затемнувачки двојки се Епсилон Кочијаш, VV Кефеј, HR 5171 и црвената џиновска двојка KIC 9246715 во соѕвездието Лебед.[1]

Список

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Напомена: Обоените редови се тела наведени за споредба.

Список на најголеми ѕвезди
Име на ѕвездата Сончеви полупречници
(Сонце = 1)		 Начин
Сатурнова орбита1.940–2.169
UY Штит1.708 ± 192[2]AD
NML Лебед1.640[3], 1.183[4]–2.770[3]L/Teff
WOH G641.540 ± 77[5]L/Teff
RW Кефеј 1.535 [6][7]L/Teff
Вестерлунд 1-26 1.530-1.580[8]L/Teff
VX Стрелец1.520[9]L/Teff
KY Лебед 1.420–2.850 [10]L/Teff
VY Големо Куче1.420 ± 120[11]AD
AH Скорпија1.411 ± 124[2]AD
VV Кефеј A 1.400[12], 1.050[13]–1.900[10]
RSGC1-F021.398[14]L/Teff
IRC+10420 (V1302 Орел)1.342[4]L/Teff
RSGC1-F011.335[14]L/Teff
HR 5171 A 1.315 ± 260[15], 1.575 ± 400[16]AD
SMC 181361.310[17]
PZ Касиопеја1.260-1.340[18] 1.190-1.940[10]L/Teff
Ми Кефеј1.260[19]
LMC 1360421.240[17]
BI Лебед1.240[10]L/Teff
SMC 50921.220[17]
S Персеј1.212 ± 124[20]AD и L/Teff
LMC 1754641.200[17]
LMC 1357201.200[17]
RAFGL 21391.200[21]
SMC 698861.190[17]
RSGC1-F051.177[14]L/Teff
EV Кобилица1.168[22]-2.880[23]L/Teff
RSGC1-F031.168[14]L/Teff
LMC 1192191.150[17]
RSGC1-F081.146[14]L/Teff
BC Лебед1.140[10]-1.230[19]L/Teff
SMC 108891.130[17]
LMC 1414301.110[17]
LMC 1757461.100[17]
RSGC1-F131.098[14]L/Teff
RT Кобилица1.090[10]L/Teff
RSGC1-F041.082[14]L/Teff
LMC 1747141.080[17]
LMC 681251.080[17]
SMC 494781.080[17]
SMC 201331.080[17]
V396 Кентаур1.070[10]L/Teff
SMC 89301.070[17]
Јупитерова орбита1.064–1.173
HV 114231.060–1.220[24]L/Teff
CK Кобилица1.060[10]L/Teff
SMC 258791.060[17]
LMC 1422021.050[17]
LMC 1461261.050[17]
LMC 679821.040[17]
U Гуштер1.022[9]L/Teff
RSGC1-F111.015[14]L/Teff
LMC 1438771.010[17]
KW Стрелец1.009[2]-1.460[10]AD и L/Teff
SMC 46497990[17]
LMC 140296990[17]
RSGC1-F09986[14]L/Teff
NR Лисица980[10]L/Teff
SMC 12322980[17]
LMC 177997980[17]
SMC 59803970[17]
GCIRS 7960 ± 92[25]AD
Бетелгез (Алфа Орион)955 ± 217[26]AD
SMC 50840950[17]
RSGC1-F10931[14]L/Teff
S Касиопеја930[27][28]
IX Кобилица920[10]L/Teff
HV 2112916[29]L/Teff
RSGC1-F07910[14]L/Teff
LMC 54365900[17]
NSV 25875891[4]L/Teff
LMC 109106890[17]
RSGC1-F06885[14]L/Teff
LMC 116895880[17]
SMC 30616880[17]
LMC 64048880[17]
V437 Штит874[4]L/Teff
V602 Кобилица860[10]-1.050[30]L/Teff и AD
V669 Касиопеја859[4]L/Teff
SMC 55681850[17]
SMC 15510850[17]
LMC 61753830[17]
LMC 62090830[17]
SMC 11709830[17]
V1185 Скорпија830[4]L/Teff
Надворешни граници на астероидниот појас816
LMC 142199810[17]
LMC 134383800[17]
BO Кобилица790[10]L/Teff
LMC 142907790[17]
SU Персеј780[10]L/Teff
RS Персеј770[31]-1.000[10]AD и L/Teff
AV Персеј770[10]L/Teff
V355 Кефеј770[10]L/Teff
V915 Скорпија760[32]L/Teff
S Кефеј760[33]
SMC 11939750[17]
HD 303250750[10]
V382 Кобилица747[34]
RU Девица742[33]
LMC 137818740[17]
SMC 48122740[17]
SMC 56732730[17]
V648 Касиопеја710[10]L/Teff
XX Персеј710[35]L/Teff
TV Близнаци620-710[36] (–770)[10]L/Teff
HD 179821704[37]
LMC 169754700[17]
LMC 65558700[17]
V528 Кобилица700[10]L/Teff
Следниве познати ѕвезди се наведени за споредба.
V354 Кефеј690[9]-1.520[10]L/Teff
Антарес A (Алфа Скорпија A)680[38]AD
CE Бик608[39]
R Зајак400–535[40]
Ро Касиопеја400-500[41]
внатрешни граници на астероидниот појас412
Мира A (Омикрон Кит)332–402[42]
V509 Касиопеја400–900[43]
CW Лав390–500[44], 700[45]–826[4]L/Teff
V838 Еднорог380 (in 2009)[46]
S Златна Рипка100-380[47]
R Златна Рипка370 ± 50[48]
Пиштол340[49]
Ла Суперба (Y Ловечки Кучиња)307[4]-390[50]L/Teff
Животопогоден појас на Сончевиот Систем305
Марсова орбита297–358
Алфа Херкул (Рас Алгети)284 ± 60[51]
црвеноџиновска фаза на Сонцето256[52]
Ета Кобилица A (Цин-ше)250[53], 60–800[54]
Земјина орбита211–219
Денеб (Алфа Лебед)203 ± 17[55]
LBV 1806-20200[56]
Венерина орбита154–157
Епсилон Кочијаш A (Алмааз)143-358[57]
WR 102ka92[58]
Ригел A (Бета Орион A)78,9[59]–115[60]
Канопус (Алфа Кобилица)71 ± 4[61]
Меркурова орбита66–100
Алдебаран (Алфа Бик)44,13 ± 0,84[62]
Северница (Алфа Голема Мечка)37,5[63]
R136a135,4[64]
Арктур (Алфа Воловар)25,4 ± 0,2[65]
HDE 22686820-22[66]
VV Кефеј B13[67]-25[68]
хелиумосогорна фаза на Сонцето10
Сонце1

Поврзано

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Наводи

[уреди | уреди извор]
  1. ↑ Hełminiak, K.G.; Ukita, N.; Kambe, E.; Konacki, M. (2015). „Absolute Stellar Parameters of KIC 09246715: A Double-giant Eclipsing System with a Solar-like Oscillator“. The Astrophysical Journal Letters. 813 (2): L25. arXiv:1509.03340. Bibcode:2015ApJ...813L..25H. doi:10.1088/2041-8205/813/2/L25.
  2. 1 2 3 Arroyo-Torres, B; Wittkowski, M; Marcaide, J. M; Hauschildt, P. H (June 2013). „The atmospheric structure and fundamental parameters of the red supergiants AH Scorpii, UY Scuti, and KW Sagittarii“. Astronomy & Astrophysics. 554 (A76): A76. arXiv:1305.6179. Bibcode:2013A&A...554A..76A. doi:10.1051/0004-6361/201220920.
  3. 1 2 Zhang, B.; Reid, M. J.; Menten, K. M.; Zheng, X. W.; Brunthaler, A. (2012). „The distance and size of the red hypergiant NML Cygni from VLBA and VLA astrometry“. Astronomy & Astrophysics. 544: A42. arXiv:1207.1850. Bibcode:2012A&A...544A..42Z. doi:10.1051/0004-6361/201219587.
  4. 1 2 3 4 5 6 7 8 De Beck, E.; Decin, L.; De Koter, A.; Justtanont, K.; Verhoelst, T.; Kemper, F.; Menten, K. M. (2010). „Probing the mass-loss history of AGB and red supergiant stars from CO rotational line profiles. II. CO line survey of evolved stars: Derivation of mass-loss rate formulae“. Astronomy and Astrophysics. 523: A18. arXiv:1008.1083. Bibcode:2010A&A...523A..18D. doi:10.1051/0004-6361/200913771.
  5. ↑ Levesque, Emily M; Massey, Philip; Plez, Bertrand; Olsen, Knut A. G (June 2009). „The Physical Properties of the Red Supergiant WOH G64: The Largest Star Known?“. Astronomical Journal. 137 (6): 4744. arXiv:0903.2260. Bibcode:2009AJ....137.4744L. doi:10.1088/0004-6256/137/6/4744.
  6. ↑ Humphreys, R. M. (1978). „Studies of luminous stars in nearby galaxies. I. Supergiants and O stars in the Milky Way“. The Astrophysical Journal Supplement Series. 38: 309. Bibcode:1978ApJS...38..309H. doi:10.1086/190559.
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  8. ↑ Wright, Nicholas J; Wesson, Roger; Drew, Janet E; Barentsen, Geert; Barlow, Michael J; Walsh, Jeremy R; Zijlstra, Albert; Drake, Jeremy J; Eislöffel, Jochen; Farnhill, Hywel J (2014). „The ionized nebula surrounding the red supergiant W26 in Westerlund 1“. Monthly Notices of the Royal Astronomical Society: Letters. 437: L1. arXiv:1309.4086. Bibcode:2014MNRAS.437L...1W. doi:10.1093/mnrasl/slt127.
  9. 1 2 3 Mauron, N.; Josselin, E. (2011). „The mass-loss rates of red supergiants and the de Jager prescription“. Astronomy and Astrophysics. 526: A156. arXiv:1010.5369. Bibcode:2011A&A...526A.156M. doi:10.1051/0004-6361/201013993.
  10. 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 Table 4 in Levesque, Emily M.; Massey, Philip; Olsen, K. A. G.; Plez, Bertrand; Josselin, Eric; Maeder, Andre; Meynet, Georges (2005). „The Effective Temperature Scale of Galactic Red Supergiants: Cool, but Not as Cool as We Thought“. The Astrophysical Journal. 628 (2): 973. arXiv:astro-ph/0504337. Bibcode:2005ApJ...628..973L. doi:10.1086/430901.
  11. ↑ Wittkowski, M.; Hauschildt, P. H.; Arroyo-Torres, B.; Marcaide, J. M. (2012). „Fundamental properties and atmospheric structure of the red supergiant VY Canis Majoris based on VLTI/AMBER spectro-interferometry“. Astronomy & Astrophysics. 540: L12. arXiv:1203.5194. Bibcode:2012A&A...540L..12W. doi:10.1051/0004-6361/201219126.
  12. ↑ Ridpath & Tirion 2001, стр. 112–113.
  13. ↑ Bauer, W. H.; Gull, T. R.; Bennett, P. D. (2008). „Spatial Extension in the Ultraviolet Spectrum of Vv Cephei“. The Astronomical Journal. 136 (3): 1312. Bibcode:2008AJ....136.1312H. doi:10.1088/0004-6256/136/3/1312.
  14. 1 2 3 4 5 6 7 8 9 10 11 12 Davies, B.; Figer, D. F.; Law, C. J.; Kudritzki, R. P.; Najarro, F.; Herrero, A.; MacKenty, J. W. (2008). „The Cool Supergiant Population of the Massive Young Star Cluster RSGC1“. The Astrophysical Journal. 676 (2): 1016–1028. arXiv:0711.4757. Bibcode:2008ApJ...676.1016D. doi:10.1086/527350.
  15. ↑ Chesneau, O.; Meilland, A.; Chapellier, E.; Millour, F.; Van Genderen, A. M.; Nazé, Y.; Smith, N.; Spang, A.; Smoker, J. V.; Dessart, L.; Kanaan, S.; Bendjoya, Ph.; Feast, M. W.; Groh, J. H.; Lobel, A.; Nardetto, N.; Otero, S.; Oudmaijer, R. D.; Tekola, A. G.; Whitelock, P. A.; Arcos, C.; Curé, M.; Vanzi, L. (2014). „The yellow hypergiant HR 5171 A: Resolving a massive interacting binary in the common envelope phase“. Astronomy & Astrophysics. 563: A71. arXiv:1401.2628v2. Bibcode:2014A&A...563A..71C. doi:10.1051/0004-6361/201322421.
  16. ↑ Wittkowski, M; Abellan, F. J; Arroyo-Torres, B; Chiavassa, A; Guirado, J. C; Marcaide, J. M; Alberdi, A; De Wit, W. J; Hofmann, K.-H; Meilland, A; Millour, F; Mohamed, S; Sanchez-Bermudez, J (28 September 2017). „Multi-epoch VLTI-PIONIER imaging of the supergiant V766 Cen: Image of the close companion in front of the primary“. 1709: arXiv:1709.09430. arXiv:1709.09430. Bibcode:2017arXiv170909430W. Наводот journal бара |journal= (help)
  17. 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 40 41 42 43 44 45 Levesque, Emily M.; Massey, Philip; Olsen, K.A.G.; Plez, Bertrand; Meynet, Georges; Maeder, Andre (2006). „The Effective Temperatures and Physical Properties of Magellanic Cloud Red Supergiants: The Effects of Metallicity“. The Astrophysical Journal. 645 (2): 1102. arXiv:astro-ph/0603596. Bibcode:2006ApJ...645.1102L. doi:10.1086/504417.
  18. ↑ Kusuno, K.; Asaki, Y.; Imai, H.; Oyama, T. (2013). „Distance and Proper Motion Measurement of the Red Supergiant, Pz Cas, in Very Long Baseline Interferometry H2O Maser Astrometry“. The Astrophysical Journal. 774 (2): 107. arXiv:1308.3580. Bibcode:2013ApJ...774..107K. doi:10.1088/0004-637X/774/2/107.
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  23. ↑ De Jager, C; Nieuwenhuijzen, H; Van Der Hucht, K. A (1988). „Mass loss rates in the Hertzsprung-Russell diagram“. Astronomy and Astrophysics Supplement Series (ISSN 0365-0138). 72: 259. Bibcode:1988A&AS...72..259D.
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  29. ↑ Levesque, Emily M.; Massey, P.; Zytkow, A. N.; Morrell, N. (1 September 2014). „Discovery of a Thorne-̇Żytkow object candidate in the Small Magellanic Cloud“. Monthly Notices of the Royal Astronomical Society: Letters. 443: L94. arXiv:1406.0001. Bibcode:2014MNRAS.443L..94L. doi:10.1093/mnrasl/slu080.
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  35. ↑ Fok, Thomas K. T.; Nakashima, Jun-Ichi; Yung, Bosco H. K.; Hsia, Chih-Hao; Deguchi, Shuji (2012). „Maser Observations of Westerlund 1 and Comprehensive Considerations on Maser Properties of Red Supergiants Associated with Massive Clusters“. The Astrophysical Journal. 760: 65. arXiv:1209.6427. Bibcode:2012ApJ...760...65F. doi:10.1088/0004-637X/760/1/65.
  36. ↑ Wasatonic, Richard P.; Guinan, Edward F.; Durbin, Allyn J. (2015). „V-Band, Near-IR, and TiO Photometry of the Semi-Regular Red Supergiant TV Geminorum: Long-Term Quasi-Periodic Changes in Temperature, Radius, and Luminosity“. Publications of the Astronomical Society of the Pacific. 127 (956): 1010. Bibcode:2015PASP..127.1010W. doi:10.1086/683261.
  37. ↑ Hawkins, G. W; Skinner, C. J; Meixner, M. M; Jernigan, J. G; Arens, J. F; Keto, E; Graham, J. R (1995). „Discovery of an Extended Nebula around AFGL 2343 (HD 179821) at 10 Microns“. Astrophysical Journal v.452. 452: 314. Bibcode:1995ApJ...452..314H. doi:10.1086/176303.
  38. ↑ Ohnaka, K; Hofmann, K.-H; Schertl, D; Weigelt, G; Baffa, C; Chelli, A; Petrov, R; Robbe-Dubois, S (2013). „High spectral resolution imaging of the dynamical atmosphere of the red supergiant Antares in the CO first overtone lines with VLTI/AMBER“. Astronomy & Astrophysics. 555: A24. arXiv:1304.4800. Bibcode:2013A&A...555A..24O. doi:10.1051/0004-6361/201321063.
  39. ↑ http://www.newforestobservatory.com/2012/07/02/the-second-reddest-star-in-the-sky-119-tauri-ce-tauri/
  40. ↑ Hofmann, K.-H.; Eberhardt, M.; Driebe, T.; Schertl, D.; Scholz, M.; Schoeller, M.; Weigelt, G.; Wittkowski, M.; Woodruff, H. C. (2005). „Interferometric observations of the Mira star o Ceti with the VLTI/VINCI instrument in the near-infrared“. Proceedings of the 13th Cambridge Workshop on Cool Stars. 560: 651. Bibcode:2005ESASP.560..651H.
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