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12CO ( 1-0 ) Molecular in Central Region of Markarian Galaxiesstatistic study | ||
| Journal of University of Anbar for Pure Science | ||
| Article 34, Volume 3, Issue 1, 2009, Pages 116-126 PDF (232.63 K) | ||
| DOI: 10.37652/juaps.2009.15504 | ||
| Author | ||
| AKRAM M. ALi | ||
| Abstract | ||
| From 2.6mm line of 12CO ( 1-0 ) molecular we utilize from data of 72 spceimens of Markarian galaxies have IR luminosity (Lfir ~ 1010L ) and inclination < i > between( 0o – 74.4o ) to investigation starformation activity from study of Hydrogen molecular ( H2 ) properties wherfrom estimation its abundunce and mass then prediction that most of molecular gas concetrate in central region of the samples , where ( CO,H2 ) look at as important tool to study galaxies structure and activities due to of staformation and its relation with other variables.Whereas most sample is late type spiral galaxies , our study emphasize that most interstellar molecular gas is ( H2 ) that can’t observed easly exept by study of CO distribution or Luminosity ( Lco ). | ||
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