subrahmanyan chandrasekhar wikipedia - EAS

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  1. Subrahmanyan Chandrasekhar - Viquipèdia, l'enciclopèdia lliure

    https://ca.wikipedia.org/wiki/Subrahmanyan_Chandrasekhar

    Subrahmanyan Chandrasekhar (tàmil: சுப்பிரமணியன் சந்திரசேகர) ( Lahore, 19 d'octubre de 1910 - Chicago, 21 d'agost de 1995 ), conegut habitualment com Chandra, fou un físic i astrònom indi guardonat amb el Premi Nobel de Física l'any 1983. [1] Biografia [ modifica]

  2. 苏布拉马尼扬·钱德拉塞卡_百度百科

    https://baike.baidu.com/item/苏布拉马尼扬·钱德拉塞卡

    苏布拉马尼扬·钱德拉塞卡(Subrahmanyan Chandrasekhar,1910年10月19日——1995年8月21日),男,印度裔美国籍物理学家和天体物理学家。钱德拉塞卡在1983年因在星体结构和进化的研究而与另一位美国天体物理学家威廉·艾尔弗雷德·福勒共同获诺贝尔物理学 ...

  3. Subrahmanyan Chandrasekhar - Vikipedi

    https://tr.wikipedia.org/wiki/Subrahmanyan_Chandrasekhar

    Chandrasekhar, 19 Ekim 1910 yılında Pencap 'ta dünyaya geldi. 10 kardeşli bir ailenin en büyük dördüncü üyesiydi. On iki yaşına kadar evde özel eğitim gören Chandrasekhar, toprak sahibi bir aileden geliyordu. Lise eğitimini 1922-25 yılları arasında Madras'ta bir Hindu Orta Okulunda yaptı. Subrahmanyan, Madras Üniversitesi 'nde eğitim gördü.

  4. Subrahmanyan Chandrasekhar – Wikipedie

    https://cs.wikipedia.org/wiki/Subrahmanyan_Chandrasekhar

    Subrahmanyan Chandrasekhar [čandrasékhár] ( 19. října 1910 Láhaur, dnes Pákistán – 21. srpna 1995 Chicago) byl americký astrofyzik a matematik indického původu. Obsah 1 Život 2 Odkazy 2.1 Reference 2.2 Související články 2.3 Externí odkazy Život [ editovat | editovat zdroj]

  5. Subrahmanyan Chandrasekhar | Space Wiki | Fandom

    https://space.fandom.com/wiki/Subrahmanyan_Chandrasekhar

    Subrahmanyan Chandrasekhar (1910 - 1995) was a Indian American Astrophysicist who mostly lived in the United States. He was was awarded the Nobel Prize for Physics in 1983 with William Alfred Fowler. He was the Best Indian American person where someone from India immigrated to USA. His uncle was CV Raman, the first Indian to win Nobel Prize.

  6. سابرامانين تشاندراسخار - ويكيبيديا

    https://ar.wikipedia.org/wiki/سابرامانين_تشاندراسخار

    كان عمه «سي. في. رامان» الفيزيائي الهندي الشهير والحائز على جائزة نوبل عام 1930. كانت والدته تكرس حياتها للسعي الفكري، فقد ترجمت بيت الدمية للكاتب المخرج المسرحي هنريك إبسن إلى اللغة التاميلية، وكانت صاحبة الفضل في إثارة الفضول الفكري لدى تشاندرا في سن مبكرة. انتقلت الأسرة من لاهور إلى «الله أباد» عام 1916، واستقرت أخيرًا في مدراس في عام 1918.

  7. Subramanyan Chandrasekhar – Biographical

    https://www.nobelprize.org/prizes/physics/1983/chandrasekhar/biographi…

    Subramanyan Chandrasekhar – Biographical - NobelPrize.org Subramanyan Chandrasekhar Biographical I was born in Lahore (then a part of British India) on the 19th of October 1910, as the first son and the third child of a family of four …

  8. Subrahmanyan Chandrasekhar

    https://starchild.gsfc.nasa.gov/docs/StarChild/whos_who_level2/chandra.html

    Subrahmanyan Chandrasekhar was born in 1910 in Lahore, which at the time was in British India. He was one of ten children born to Sita Balakrishnan and Chandrasekhara Subrahmanya Ayyar. His father was a government officer while his mother was a highly intellectual woman that translated literary works into Tamil, an Indian dialect.

  9. Subrahmanyan Chandrasekhar - Department of Physics

    https://phys-astro.sonoma.edu/brucemedalists/subrahmanyan-chandrasekhar

    S. Chandrasekhar was born in Lahore, India (now Pakistan) and received his B.A. at the University of Madras. At the University of Cambridge he earned his Ph.D. under noted physicist R.H. Fowler and developed the theory of white dwarf stars, showing that quantum mechanical degeneracy pressure cannot stabilize a massive star.

  10. Chandrasekhar's white dwarf equation - Wikipedia

    https://en.wikipedia.org/wiki/Chandrasekhar's_white_dwarf_equation

    Chandrasekhar's white dwarf equation. In astrophysics, Chandrasekhar's white dwarf equation is an initial value ordinary differential equation introduced by the Indian American astrophysicist Subrahmanyan Chandrasekhar, [1] in his study of the gravitational potential of completely degenerate white dwarf stars. The equation reads as [2]

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