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<p>one should take  equal to 2 for such a star, leading to the commonly quoted value of . (Near the beginning of the 20th&nbsp;century, there was reason to believe that stars were composed chiefly of heavy elements, so, in his 1931 paper, Chandrasekhar set the average molecular weight per electron, , equal to 2.5, giving a limit of .) Together with <a href="page.php?w=William_Alfred_Fowler">William Alfred Fowler</a>, Chandrasekhar received the <a href="page.php?w=Nobel_Prize_in_Physics">Nobel Prize</a> for this and other work in 1983. The limiting</p><p>
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