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قائمة أكبر النجوم: الفرق بين النسختين

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سطر 30:
! style="background:#efefef; white-space:nobr;width:8em"| النجم|| [[نصف قطر شمسي]]<br />([[الشمس]] = 1)
|-
|[[آر دبليو الملتهب]]
| [[يو واي سكوتي]] || '''1,708 ± 192'''<ref name="torres2013">{{Cite journal | last1 = Arroyo-Torres | first1 = B. | last2 = Wittkowski | first2 = M. | last3 = Marcaide | first3 = J. M. | last4 = Hauschildt | first4 = P. H. | title = The atmospheric structure and fundamental parameters of the red supergiants AH Scorpii, UY Scuti, and KW Sagittarii | doi = 10.1051/0004-6361/201220920 | journal = Astronomy & Astrophysics | volume = 554 | pages = A76 | year = 2013 | pmid = | pmc = | bibcode = 2013A&A...554A..76A |arxiv = 1305.6179 }}</ref>
|-
| '''[[دبليويو أوواي إتش جي 64سكوتي]] A''' || '''1,635 ± 5%'''<ref name="Levesque2009">{{cite journal
|title=The Physical Properties of the Red Supergiant WOH G64: The Largest Star Known?
|journal=Astronomical Journal
السطر 41 ⟵ 42:
|arxiv = 0903.2260 }}</ref><ref name=ohnaka>{{Cite journal | last1 = Ohnaka | first1 = K. | last2 = Driebe | first2 = T. | last3 = Hofmann | first3 = K. H. | last4 = Weigelt | first4 = G. | last5 = Wittkowski | first5 = M. | title = Resolving the dusty torus and the mystery surrounding LMC red supergiant WOH G64 | doi = 10.1017/S1743921308028858 | journal = Proceedings of the International Astronomical Union | volume = 4 | pages = 454 | year = 2009 | pmid = | pmc = | bibcode = 2009IAUS..256..454O }}</ref>
|-
| '''[[آردبليو أو إتش جي 64|دبليو الملتهبأو إتش جي64]]''' ||'''{{nobr| 1,535}}'''<ref name=humphreys>{{cite journal|doi=10.1086/190559|title=Studies of luminous stars in nearby galaxies. I. Supergiants and O stars in the Milky Way|journal=The Astrophysical Journal Supplement Series|volume=38|pages=309|year=1978|last1=Humphreys|first1=R. M.|bibcode=1978ApJS...38..309H}}</ref><ref name=davies>{{cite journal|doi=10.1111/j.1365-2966.2010.16965.x|title=The potential of red supergiants as extragalactic abundance probes at low spectral resolution|journal=Monthly Notices of the Royal Astronomical Society|volume=407|issue=2|pages=1203|year=2010|last1=Davies|first1=Ben|last2=Kudritzki|first2=Rolf-Peter|last3=Figer|first3=Donald F.|bibcode=2010MNRAS.407.1203D|arxiv = 1005.1008 }}</ref>
|-
|'''[[وسترلاند 1-26]]''' || '''1,530'''<ref name=wright>{{cite journal|last1=Wright|first1=N. J.|last2=Wesson|first2=R.|last3=Drew|first3=J. E.|last4=Barentsen|first4=G.|last5=Barlow|first5=M. J.|last6=Walsh|first6=J. R.|last7=Zijlstra|first7=A.|last8=Drake|first8=J. J.|last9=Eisloffel|first9=J.|last10=Farnhill|first10=H. J.|title=The ionized nebula surrounding the red supergiant W26 in Westerlund 1|journal=Monthly Notices of the Royal Astronomical Society: Letters|date=16 October 2013|volume=437|issue=1|pages=L1–L5|doi=10.1093/mnrasl/slt127|arxiv = 1309.4086 |bibcode = 2014MNRAS.437L...1W }}</ref>
السطر 53 ⟵ 54:
 
 
| [[الراقص (الملتهب)|رجل الجبار]] || 1,650<ref name=levesqueetal2005/>
 
|-
| [[الرامي كي دبليو|كي دبليو الرامي]] || 1,460<ref name=levesqueetal2005>Table 4 in {{Cite journal|title=The Effective Temperature Scale of Galactic Red Supergiants: Cool, but Not As Cool As We Thought |author=Emily M. Levesque, Philip Massey, K. A. G. Olsen, Bertrand Plez, Eric Josselin, Andre Maeder, and Georges Meynet |journal=The Astrophysical Journal |volume=628 |issue=2 |تاريخ=أغسطس 2005 |pages=973–985 |doi=10.1086/430901 |bibcode=2005ApJ...628..973L}}</ref>
|
 
|-
| [[منكبقلب الجوزاءالعقرب (نجم)]] || 1,180<ref>{{Cite journal|author=Graham M. Harper et al |year=2008 |journal=The Astronomical Journal |volume=135 |pages=1430–1440 |doi=10.1088/0004-6256/135/4/1430 |bibcode=2008AJ....135.1430H}}</ref><ref>Jim Kaler. 2009-06-26. [http://www.astro.uiuc.edu/~kaler/sow/betelgeuse.html Betelgeuse ] "0.047 seconds of arc, from which we find a true radius of between 4.1 (compromise distance) and 4.6 (larger distance) AU, … extended atmosphere, and the pulsations make it difficult to locate an actual "surface" to tell just how large the star actually is. … "size" of the star depends on the color of observation. Long-wave infrared … up to 5 AU and greater, … shorter-wave infrared … 3 AU. … Betelgeuse to be shrinking … not even round, but somewhat oval"</ref>
|-
| [[في في الملتهب|في في الملتهب أ]] ||'''1,050'''<ref name=bauer2008>{{Cite journal | last1 = Bauer | first1 = W. H. | last2 = Gull | first2 = T. R. | last3 = Bennett | first3 = P. D. | doi = 10.1088/0004-6256/136/3/1312 | title = Spatial Extension in the Ultraviolet Spectrum of Vv Cephei | journal = The Astronomical Journal | volume = 136 | issue = 3 | pages = 1312 | year = 2008 | pmid = | pmc = |bibcode = 2008AJ....136.1312H }}</ref>
|-
| [[قلب العقرب (نجم)|منكب الجوزاء]] || 800<ref group="foot">approximately 800, derived from the 1990 lunar occultation measurement of apparent diameter of 43.1 milliarcsec (up to ±1 milliarcsec error) (http://adsabs.harvard.edu/abs/1990A&A...230..355R page 361) together with 1997 parallax of 5.40 [1.68] milliarcsec ([http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=Antares&submit=SIMBAD+search SIMBAD] citing [http://astrobib.u-strasbg.fr:2008/cgi-bin/cdsbib?1997A&A...323L..49P Hipparcos]). The parallax gives a derived distance from 460 to 877 light years. This in turn yields an actual diameter from 653 to 1,246 solar radius. An average of 800 is used here.</ref>
|-
| [[في 382 القاعدة]] || 747
السطر 142 ⟵ 143:
| غاما المرأة المسلسلة|| 83
|-
| [[رجلالراقص الجبار(الملتهب)]] || 78
|-
| [[الأرنب (نجم)]] ''(Arneb)'' || 77
مجلوبة من «https://ar.wikipedia.org/wiki/قائمة_أكبر_النجوم»