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Stars, Dust and Nebula in NGC 2170
<< Yesterday 27.02.2007 Tomorrow >>
Stars, Dust and Nebula in NGC 2170
Credit & Copyright: Russell Croman (Russell Croman Astrophotography)
Explanation: When stars form, pandemonium reigns. A textbook case is the star forming region NGC 2170. Visible above are red glowing emission nebulas of hydrogen, blue reflection nebulas of dust, dark absorption nebulas of dust, and the stars that formed from them. The first massive stars formed from the dense gas will emit energetic light and winds that erode, fragment, and sculpt their birthplace. And then they explode. The resulting morass is often as beautiful as it is complex. After tens of millions of years, the dust boils away, the gas gets swept away, and all that is left is a naked open cluster of stars.

<<  Fevral'  >>
Pn Vt Sr Cht Pt Sb Vs
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12 13 14 15 16 17 18
19 20 21 22 23 24 25
26 27 28        
1995   1996   1997   1998
1999   2000   2001   2002
2003   2004   2005   2006
2007   2008   2009   2010
2011   2012   2013   2014
2015   2016   2017   2018
2019   2020   2021   2022
2023   2024   2025  
Yanvar'
Fevral'
Mart
Aprel'
Mai
Iyun'
Iyul'
Avgust
Sentyabr'
Oktyabr'
Noyabr'
Dekabr'
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.

Russkii tekst
Based on Astronomy Picture Of the Day
Publikacii s klyuchevymi slovami: reflection nebula - emission nebula - otrazhatel'nye tumannosti - emissionnaya tumannost'
Publikacii so slovami: reflection nebula - emission nebula - otrazhatel'nye tumannosti - emissionnaya tumannost'
Sm. takzhe:
Vse publikacii na tu zhe temu >>

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