आकाशगंगा: रिवीजन सभ के बीचा में अंतर
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लाइन 20:
| data7 = ≥13.7 [[Byr|Gyr]]<ref name=HD_140283_(arXiv)>{{cite journal |title=HD 140283: A Star in the Solar Neighborhood that Formed Shortly After the Big Bang |date=February 13, 2013 |author1=H.E. Bond |display-authors=4 |author2=E. P. Nelan |author3=D. A. VandenBerg |author4=G. H. Schaefer |author5=D. Harmer |doi=10.1088/2041-8205/765/1/L12 |journal=The Astrophysical Journal |volume=765 |pages=L12 |issue=1 |arxiv=1302.3180|bibcode = 2013ApJ...765L..12B }}</ref>
| label8 = द्रब्यमान
| data8 = 0.8–1.5{{e|12}} {{solar mass|link=yes}}<ref name=McMillan2011>{{Cite journal | last1 = McMillan | first1 = P. J. | title = Mass models of the Milky Way | doi = 10.1111/j.1365-2966.2011.18564.x | journal = Monthly Notices of the Royal Astronomical Society | volume = 414 | issue = 3 | pages = 2446–2457 | date=July 2011 | bibcode=2011MNRAS.414.2446M| pmid = | pmc = |arxiv = 1102.4340 }}</ref><ref name=
| label9 = कोणीय वेग
| data9 = ≈{{val|1|e=67|u=J s}}<ref>{{cite web|last1=Karachentsev|first1=Igor|title=Double Galaxies §7.1|url=https://ned.ipac.caltech.edu/level5/Sept02/Keel/Keel7.html|website=ned.ipac.caltech.edu|publisher=Izdatel'stvo Nauka|accessdate=5 अप्रैल 2015}}</ref>
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