Molecular Gas in the Central Regions of Barred Galaxies
1996 ◽
Vol 157
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pp. 150-156
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Keyword(s):
AbstractThe morphology and kinematics of molecular gas in the central regions of barred galaxies are described. The largest gas concentrations are often located near ILRs, although there is a range of morphologies. The gas motions associated with star-forming rings are predominantly circular, while motions just beyond the rings are often non-circular and in some cases show clear radial inflow. In barred galaxies with circumnuclear starbursts in early phases of evolution, the CO is centrally peaked, perhaps inside IILRs. The most intense star formation occurs where the gas motions are circular, and where the rotation curve rises steeply and is nearly solid body.
2020 ◽
Vol 498
(1)
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pp. L66-L71
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2019 ◽
Vol 488
(3)
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pp. 3904-3928
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2016 ◽
Vol 11
(S321)
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pp. 214-216
Keyword(s):
2020 ◽
Vol 495
(4)
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pp. 3840-3858
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Keyword(s):
2019 ◽
Vol 493
(2)
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pp. 2872-2909
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Keyword(s):
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2020 ◽
Vol 492
(2)
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pp. 2973-2995
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