2003
DOI: 10.1051/0004-6361:20021701
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The cold gas properties of Markarian galaxies

Abstract: Abstract.A sample of 61 Markarian galaxies detected in the CO line was compiled. Using available HI, H 2 , optical and radio continuum data, the analysis of the gas kinematics and the star formation properties for this sample of galaxies was performed. The main conclusion can be summarized as follows:(1) The HI and CO line widths are well correlated. Interaction between galaxies has no influence on the CO line broadening. A rapidly rotating nuclear disk in the galaxy might lead to the CO line broadening with l… Show more

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Cited by 20 publications
(23 citation statements)
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“…The type Ic SN2002jj (Foley & Filippenko 2002) is positioned very close to the nuclear region. Kandalyan (2003) this galaxy is a strong source of neutral HI and molecular H 2 , and CO emissions and a source of 1.4 GHz continuum radio emission (Condon et al 1998). Our morphological study confirms the Sa spiral structure of this object.…”
Section: The Morphological Classificationmentioning
confidence: 96%
“…The type Ic SN2002jj (Foley & Filippenko 2002) is positioned very close to the nuclear region. Kandalyan (2003) this galaxy is a strong source of neutral HI and molecular H 2 , and CO emissions and a source of 1.4 GHz continuum radio emission (Condon et al 1998). Our morphological study confirms the Sa spiral structure of this object.…”
Section: The Morphological Classificationmentioning
confidence: 96%
“…They derive for either galaxy a neutral gas mass M HI ∼ 5 × 10 9 M . A subsequent work of Kandalyan (2003), taking into account radio CO line observations, indicates that NGC 7679 possesses a comparable amount of molecular hydrogen (M H2 ∼ 6 × 10 9 M ).…”
Section: Radio Observationsmentioning
confidence: 97%
“…Since the CO gas kinematics reveals the rotation and/or velocity dispersion close to the nucleus, this phenomenon is interpreted as due to a rapidly rotating nuclear disk (cf. Kandalyan 2003). As such, part of this circumnuclear gas is likely prone to streaming inward with velocities ∼100 km s −1 directly onto the nucleus (cf.…”
Section: Ngc 7679 In the Framework Of The Agn-starburst Connection Issuementioning
confidence: 99%
“…c Absolute K-band magnitude (Rothberg & Joseph 2004). d Total mass of neutral atomic hydrogen gas, taken from compilation by Kandalyan (2003). e Total star formation rate (U et al 2012).…”
Section: Ngc 1614 and Ngc 34: A Tale Of Two Lirgsmentioning
confidence: 99%