Документ взят из кэша поисковой машины. Адрес оригинального документа : http://zebu.uoregon.edu/messier/m51.txt Дата изменения: Sat Apr 23 02:49:29 1994 Дата индексирования: Mon Oct 1 21:28:35 2012 Кодировка: Поисковые слова: accretion disk

M51 is another very High Surface Brightness galaxy. It is
interacting with a small companion galaxy. That interaction serves
to redistribute and compress the gas which facilitates star
formation. In addition, the symmetry of tidal encounters often
induces spiral structure in the more massive of the two galaxies.
This spiral structure is clearly seen in this blue image. M51 is
the host galaxy for SN 1994 I.