Galaxies with f12 &gt; f25

Kandalian, R. A.

doi:10.1007/bf02045330

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1999

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“…Our original sample of Mkn-IRAS galaxies contains 155 objects (Kandalian et al 1995). In order to investigate the gas properties of Mkn-IRAS galaxies in our sample we have extracted from the literature all objects which were detected in the 12CO(1-0) line (till July, 1997).…”

Section: Resultsmentioning

confidence: 99%

Gas Content of Markarian Starburst Galaxies

Kandalyan¹

1999

Symp. - Int. Astron. Union

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The main results of this study can be summarized as follows: (a) The HI and CO linewidths are well correlated. Interaction between galaxies has little influence on the HI and CO line broadening. A rapidly rotating nuclear disk in the galaxy could lead to CO line broadening, while the HI line is less affected by the rotating disk. Molecular gas in Markarian galaxies is centrally concentrated. (b) For past and present star formation activity both HI and H2 components of the gas are important. The atomic and molecular gas surface densities are well correlated with blue, FIR, and radio continuum surface brightnesses, but the H2 surface density is better correlated than that of the HI. The two gas phases are also connected. (c) In general, galaxies with UV-excess (Markarian galaxies) are not distinguished by star formation properties from non-UV galaxies, however some second order differences may exist, like the relation between atomic surface density and radio continuum surface brightness.

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Section: Resultsmentioning

confidence: 99%

Gas Content of Markarian Starburst Galaxies

Kandalyan¹

1999

Symp. - Int. Astron. Union

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Galaxies with f12 > f25

Cited by 1 publication

References 11 publications

Gas Content of Markarian Starburst Galaxies

Gas Content of Markarian Starburst Galaxies

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