Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.astronet.ru/db/xware/msg/apod/1995-12-31
Дата изменения: Sat Oct 5 11:39:30 2002
Дата индексирования: Mon Feb 4 11:26:14 2013
Кодировка:
LMC X-1: A Black Hole Candidate
Astronomy Picture of the Day
    


LMC X-1: A Black Hole Candidate
<< Yesterday 29.12.1995 Tomorrow >>
LMC X-1: A Black Hole Candidate
Credit & Copyright: ROSAT, MPE, NASA
Explanation: The strongest source of X-rays in the Large Magellanic Cloud originates from an unusually energetic binary star system. This strong source, dubbed LMC X-1, is thought to be a normal and compact star orbiting each other. Gas stripped of the normal star falls onto the compact star, heats up, and emits X-rays. The X-rays shining from the system knock electrons off atoms for light years around, causing some atoms to glow noticeably in X-rays when the electrons re-combine. Motion in the binary system indicates the compact star is probably a black hole, since its high mass - roughly five times that of our Sun - should be enough to cause even a neutron star to implode.

January
February
March
April
May
June
July
August
September
October
November
December
 < December 1995  >
Mo Tu We Th Fr Sa Su




123
45678910
11121314151617
18192021222324
25262728293031
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.

Based on Astronomy Picture Of the Day

Publications with keywords: black hole - LMC
Publications with words: black hole - LMC
See also:
All publications on this topic >>