Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.astronet.ru/db/varstars/msg/1198707
Дата изменения: Thu Jul 15 10:15:32 2004
Дата индексирования: Sat Feb 12 19:12:50 2011
Кодировка:
Journal "Peremennye Zvezdy"
Peremennye Zvezdy

Stars and Dust in Corona Australis
<< Yesterday 15.07.2004 Tomorrow >>
Stars and Dust in Corona Australis
Credit & Copyright: Loke Kun Tan (StarryScapes)
Explanation: A cosmic dust cloud sprawls across a rich field of stars in this gorgeous wide field telescopic vista looking toward Corona Australis, the Southern Crown. Probably less than 500 light-years away and effectively blocking light from more distant, background stars in the Milky Way, the densest part of the dust cloud is about 8 light-years long. At its tip (lower left) are a series of lovely blue nebulae cataloged as NGC 6726, 6727, and 6729. Their characteristic blue color is produced as light from hot stars is reflected by the cosmic dust. The tiny but intriguing yellowish arc visible near the blue nebulae marks young variable star R Corona Australis. Magnificent globular star cluster NGC 6723 is seen here below and left of the nebulae. While NGC 6723 appears to be just outside Corona Australis in the constellation Sagittarius, it actually lies nearly 30,000 light-years away, far beyond the Corona Australis dust cloud.

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

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