Subramanyan Chandrasekhar - Autobiography Subramanyan Chandrasekhar Autobiography. I was born in Lahore (then a part of British India) on the 19th of October 1910, as the first son and http://tmsyn.wc.ask.com/r?t=an&s=hb&uid=24312681243126812&sid=343126
Chandrasekhar, Subramanyan Brief biography and details of his scientific animosity with Eddington. (Author Eric W. Weisstein) http://tmsyn.wc.ask.com/r?t=an&s=hb&uid=24312681243126812&sid=343126
Subrahmanyan Chandrasekhar Subramanyan Chandrasekhar Chandrasekhar was born in Lahore, British India (now Pakistan). He died in Chicago, Illinois, USA . See also Chandrasekhar limit http://tmsyn.wc.ask.com/r?t=an&s=hb&uid=24312681243126812&sid=343126
Chandrasekhar, Subramanyan Chandrasekhar, Subramanyan (19101995) Je suis n dans Lahore (alors une partie de l'Inde Britannique) le 19 octobre 1910, comme le premier fils et http://tmsyn.wc.ask.com/r?t=an&s=hb&uid=24312681243126812&sid=343126
Subrahmanyan Chandrasekhar Subramanyan Chandrasekhar Subrahmanyan Chandrasekhar Subramanyan Chandrasekhar. Subrahmanyan Chandrasekhar (October 19, 1910 August 21, 1995) was an Indian physicist http://tmsyn.wc.ask.com/r?t=an&s=hb&uid=24312681243126812&sid=343126
Subrahmanyan Chandrasekhar Subramanyan Chandrasekhar (19101995). Born in Lahore, India, in 1910, theoreticalastrophysicist Chandrasekhar was elected to the Academy only two years http://www7.nationalacademies.org/archives/chandra.html
Extractions: Subrahmanyan Chandrasekhar University of Chicago photograph Subramanyan Chandrasekhar (1910-1995). Born in Lahore, India, in 1910, theoretical astrophysicist Chandrasekhar was elected to the Academy only two years after he became a US citizen in 1953. Chandrasekhar was noted for his work in the field of stellar evolution, and in the early 1930s he was the first to theorize that a collapsing massive star would become an object so dense that not even light could escape it. Although this finding was greeted with some skepticism at the time it was announced, it went on to form the foundation of the theory of black holes, and eventually earned Chandrasekhar a shared Nobel Prize in physics for 1983. In addition to his work on star degeneration, Chandrasekhar contributed important theorems on the stability of cosmic masses in the presence of gravitation, rotation, and magnetic fields; this work proved to be crucial for the understanding of the spiral structure of galaxies. From the time he came to the US in 1936 until his death in 1995, Chandrasekhar was affiliated with the University of Chicago and its Yerkes Observatory. Subscribe to e-newsletters Feedback Back to Top
The Nobel Prize In Physics 1983: Subramanyan Chandrasekhar Subramanyan Chandrasekhar *1910 1995 The Nobel Prize in Physics 1983Subramanyan Chandrasekhar *1910 1995. External links http://www.nobelpreis.org/english/physik/chandrasekhar.htm
Physicist / Astronomer C chandrasekhar subramanyan. Born 19 Oct 1910 in Lahore, India (now Pakistan)Died 21 Aug 1995 in Chicago, Illinois, USA. 1983 Nobel Physics prize for his http://www.mlahanas.de/Stamps/Data/PHPerson/C.htm
Extractions: More a mathematician, Carnot's interests in his last years turned toward the steam engine with the first steam engine coming to Magdeburg in 1818. His son Sadi Carnot visited him in Magdeburg in 1821 and it is clear that Lazare Carnot influenced his son. Sadi Carnot published his masterpiece on the thermodynamics of the steam engine three years later Celsius was born in Uppsala, one of a large number of scientists (all related) originating from Ovanåker in the province of Hälsingland. The family name is a latinised version of the name of the vicarage (Högen). His grandfathers were both professors in Uppsala: Magnus Celsius the mathematician and Anders Spole the astronomer. His father, Nils Celsius, was also professor in astronomy. Celsius, who was said to have been very talented in mathematics from an early age, was appointed professor of astronomy in 1730. He began his "grand tour", lasting for four years, in 1732, and he visited during these years almost all the notable european observatories of the day, where he worked with many of the leading 18th century astronomers.
Extractions: Died : 1995 Subrahmanyan Chandrasekhar, a Nobel Laureate in Physics and one of the greatest astrophysicists of modern times was born on October 19, 1910 in Lahore, (now in Pakistan) to parents Chandrasekhara Subrahmanya Ayyaa civil servant and Sita Balakrishnan. Being the nephew of the great, C.V. Raman , a Nobel Prize winner in Physics young Chandrashekhar's interest in the subject came naturally to him. In 1930, at the age of 19, he completed his degree in Physics from Presidency College, Madras and went to England for postgraduate studies at the Cambridge University. Chandrasekhar was noted for his work in the field of stellar evolution, and in the early 1930s he was the first to theorize that a collapsing massive star would become an object so dense that not even light could escape it; now known as the Black hole. He demonstrated that there is an upper limit ( known as 'Chandrasekhar Limit' ) to the mass of a White dwarf star. His theory challenged the common scientific notion of the 1930s that all stars, after burning up their fuel, became faint, planet-sized remnants known as white dwarfs. But today, the extremely dense neutron stars and black holes implied by Chandrasekhars early work are a central part of the field of astrophysics. Initially his theory was rejected by peers and professional journals in England. The distinguished astronomer Sir Arthur Eddington publicly ridiculed his suggestion that stars could collapse into such objects( black holes). Disappointed, and reluctant to engage in public debate, Chandrasekhar moved to America and in 1937 joined the faculty as an Assistant Professor of Astrophysics at the University of Chicago and remained there till his death. At Chicago, he immersed himself in a personalized style of research and teaching, tackling first one field of astrophysics and then another in great depth. He wrote more than half a dozen definitive books describing the results of his investigations. More than 100,000 copies of his highly technical books have been sold. He also served as editor of the Astrophysical Journal, the fields leading journal, for nearly 20 years; presided over a thousand colloquia; and supervised Ph.D. research for more than 50 students.
Subramanyan Chandrasekhar SUBRAMANYAN CHANDRASEKHAR. 10. 10. 1910 1995. indický fyzik. Byl nejstarí zosmi detí. Fyziku zacal studovat na univerzite v roce 1927. http://vedci.wz.cz/Osobnosti/Chandrasekhar_S.htm
Extractions: indický fyzik Byl nejstarí z osmi dìtí. Fyziku zaèal studovat na univerzitì v roce 1927. Bìhem studia ho zaujaly práce o bílých trpaslících, tìlesech povaovaných v té dobì za koneèný stupeò vývoje hvìzd. V osmnácti letech mu velmi významný vìdecký èasopis uveøejnil èlánek a to mu otevøelo cestu ke studiu na univerzitì v Cambridge. Indii opustil v roce 1930. Jakmile se mu podaøilo pøekonat moøskou nemoc, vzpomnìl si na bílé trpaslíky. Napadlo jej, e by mohl spojit teorii i bílých trpaslících a speciální teorii relativity. Výsledky jej pøekvapily. Doel k závìru, e bílí trpaslíci nejsou jedinou monou závìreènou fází vývoje hvìzd. Na pøednáce jeho teorii odmítl pøední britský astronom Sir A. Eddington. Trvalo nìkolik desítek let, ne teorie byla pøijata. Roku 1983 za ni byl odmìnìn Nobelovou cenou za fyziku. A B C D ... Z
Subramanyan Chandrasekhar - Wikipedia Subramanyan Chandrasekhar. Subramanyan Chandrasekhar (19 oktober 1910 21 augustus1995) is een van oorsprong Indiaas theoretisch natuurkundige. http://nl.wikipedia.org/wiki/Subramanyan_Chandrasekhar
Extractions: Subramanyan Chandrasekhar 19 oktober 21 augustus ) is een van oorsprong Indiaas theoretisch natuurkundige . Hij toonde in aan dat sterren met een massa groter dan 1,4 maal die van de zon ineen zouden storten tot objecten met een enorme dichtheid. Objecten met zo'n enorme zwaartekracht dat zelfs het licht niet zou kunnen ontsnappen. Zijn ontdekking werd met de nodige skepsis bekeken, maar tegenwoordig weten we dat dat neutronensterren en zwarte gaten zijn. De massa van 1,4 maal de zonmassa wordt ook wel de Chandrasekhar-limiet genoemd. Als de massa minder is dan 1,4 zonmassa's, dan eindigt een ster als witte dwerg . Voorbeelden van witte dwergen: Sirius B en O2 Eridani B. Chandrasekhar kreeg hiervoor in de Nobelprijs voor de Natuurkunde . Hij droeg verder bij aan het begrip van de stabiliteit van grote kosmische structuren, zoals spiraalstelsels. Chandrasekhar werd geboren in Lahore , destijds in Brits India (nu Pakistan ). Hij overleed in Chicago Illinois VS . De Chandra X-Ray Observatory is naar hem vernoemd. Categorie«n Indiaas wetenschapper Natuurkundige Astronoom Views Persoonlijke instellingen Navigatie Informatie Zoeken hulpmiddelen in andere talen Äesky Deutsch English Espa±ol ... Svenska De laatste wijziging op deze pagina vond plaats op 14 sep 2005 21:08.
Subramanyan Chandrasekhar Subramanyan Chandrasekhar. Subrahmanyan Chandrasekhar (ur. 19 pazdziernika1910, zm. 21 sierpnia 1995) byl hinduskim astrofizykiem i matematykiem. http://encyklopedia.servis.pl/wiki/Subramanyan_Chandrasekhar
Extractions: Subrahmanyan Chandrasekhar (ur. 19 października , zm. 21 sierpnia ) byÅ hinduskim astrofizykiem i matematykiem . WiÄkszÄ czÄÅÄ Å¼ycia spÄdziÅ w USA , pracujÄ c na Uniwersytecie w Chicago W otrzymaÅ NagrodÄ Nobla z fizyki za wykonane na samym poczÄ tku kariery naukowej obliczenia, wykazujÄ ce istnienie maksymalnej możliwej masy biaÅego karÅa Granica Chandrasekhara Na jego czeÅÄ nazwano wystrzelony przez NASA w kosmiczny kosmiczny teleskop rentgenowski Chandra
Extractions: Subramanyan Chandrasekhar , f¶dd 19 oktober i Lahore Indien , d¶d 21 augusti . Amerikansk nobelpristagare i fysik . Han fick priset med motiveringen " f¶r hans teoretiska studier av de fysikaliska processer, som ¤r av betydelse f¶r stj¤rnornas struktur och utveckling ". Han delade priset med William A Fowler redigera Den h¤r artikeln ¤r h¤mtad fr¥n http://sv.wikipedia.org/wiki/Subramanyan_Chandrasekhar Artikelkategorier Nobelpristagare i fysik Visningar Personliga verktyg Navigering S¶k Verktygsl¥da Andra spr¥k Äesky Deutsch English Espa±ol ... SlovenÅ¡Äina Den h¤r sidan ¤ndrades senast 25 juli 2005 kl.06.34. All text tillg¤nglig under GNU Free Documentation License Om Wikipedia F¶rbeh¥ll
Subramanyan Chandrasekhar - Wikipedia, Wolna Encyklopedia Subramanyan Chandrasekhar. Z Wikipedii, wolnej encyklopedii. SubrahmanyanChandrasekhar (ur. 19 pazdziernika 1910, zm. 21 sierpnia 1995) byl hinduskim http://pl.wikipedia.org/wiki/Subramanyan_Chandrasekhar
Extractions: Subrahmanyan Chandrasekhar (ur. 19 października , zm. 21 sierpnia ) byÅ hinduskim astrofizykiem i matematykiem . WiÄkszÄ czÄÅÄ Å¼ycia spÄdziÅ w USA , pracujÄ c na Uniwersytecie w Chicago W otrzymaÅ NagrodÄ Nobla z fizyki za wykonane na samym poczÄ tku kariery naukowej obliczenia, wykazujÄ ce istnienie maksymalnej możliwej masy biaÅego karÅa Granica Chandrasekhara Na jego czeÅÄ nazwano wystrzelony przez NASA w kosmiczny kosmiczny teleskop rentgenowski Chandra Źr³dÅo: " http://pl.wikipedia.org/wiki/Subramanyan_Chandrasekhar Kategorie ZalÄ Å¼ki artykuųw - astronomia NobliÅci - fizyka ... Hindusi Views osobiste nawigacja Szukaj narzÄdzia W innych jÄzykach Äesky Deutsch English Espa±ol ... Svenska TÄ stronÄ ostatnio zmodyfikowano o 06:31, 25 lip 2005 TreÅÄ udostÄpniana na licencji GNU Free Documentation License O Wikipedii Informacje prawne
Subramanyan Chandrasekhar - Wikipedia, Wolna Encyklopedia Subramanyan Chandrasekhar. Z Wikipedii, wolnej encyklopedii. (Przekierowano zSubrahmanyan Chandrasekhar). Subrahmanyan Chandrasekhar (ur. http://pl.wikipedia.org/wiki/Subrahmanyan_Chandrasekhar
Extractions: (Przekierowano z Subrahmanyan Chandrasekhar Subrahmanyan Chandrasekhar (ur. 19 października , zm. 21 sierpnia ) byÅ hinduskim astrofizykiem i matematykiem . WiÄkszÄ czÄÅÄ Å¼ycia spÄdziÅ w USA , pracujÄ c na Uniwersytecie w Chicago W otrzymaÅ NagrodÄ Nobla z fizyki za wykonane na samym poczÄ tku kariery naukowej obliczenia, wykazujÄ ce istnienie maksymalnej możliwej masy biaÅego karÅa Granica Chandrasekhara Na jego czeÅÄ nazwano wystrzelony przez NASA w kosmiczny kosmiczny teleskop rentgenowski Chandra Źr³dÅo: " http://pl.wikipedia.org/wiki/Subramanyan_Chandrasekhar Kategorie ZalÄ Å¼ki artykuųw - astronomia NobliÅci - fizyka ... Hindusi Views osobiste nawigacja Szukaj narzÄdzia W innych jÄzykach Äesky Deutsch English Espa±ol ... Svenska TÄ stronÄ ostatnio zmodyfikowano o 06:31, 25 lip 2005
