Explanation: On August 21, 1995 one of the greatest astrophysicists of modern times passed away. Subrahmanyan Chandrasekhar was a creative, prolific genius whose ability to combine mathematical precision with physical insight changed humanity's view of stellar physics. His most famous discovery was that not all stars end up as white dwarf stars, but those retaining mass above a certain limit - today known as "Chandrasekhar's limit," undergo further collapse. His detailed mathematical papers and books on a wide variety of astrophysical subjects, including, for example, black holes, are classic references for research at every level. Obituaries are available from the University of Chicago Press and Reuters News Service, and a WWW page has been set-up to record personal memories.

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Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (USRA)
NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.

Publikacii s klyuchevymi slovami: Subrahmanyan Chandrasekhar - chernye dyry - predel Chandrasekara - Evolyuciya zvezd Publikacii so slovami: Subrahmanyan Chandrasekhar - chernye dyry - predel Chandrasekara - Evolyuciya zvezd
Sm. takzhe: Porfirion: samyi dlinnyi dzhet ot chernoi dyry Tumannost' Tyul'pan i chernaya dyra Lebed' X-1 Chernaya dyra razrushaet zvezdu: animaciya Sliyanie dvuh chernyh dyr: modelirovanie Galaktika, dzhet i znamenitaya chernaya dyra Akkrecionnyi disk chernoi dyry: vizualizaciya Akkreciruyushaya chernaya dyra s dzhetom Vse publikacii na tu zhe temu >>