12CO ( 1-0 ) Molecular in Central Region of Markarian Galaxiesstatistic study
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...
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| Format: | Article |
| Language: | English |
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University of Anbar
2009-04-01
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| Series: | مجلة جامعة الانبار للعلوم الصرفة |
| Online Access: | https://juaps.uoanbar.edu.iq/article_15504_fdc778949f5bc60b092d5104db121ac8.pdf |
| Summary: | 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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| ISSN: | 1991-8941 2706-6703 |