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VALES VII. Molecular and ionized gas properties in the pressure balanced interstellar medium of starburst galaxies at z ∼ 0.15
(European Southern Observatory, 2020)
Context. Spatially resolved observations of the ionized and molecular gas are critical for understanding the physical processes that govern the interstellar medium (ISM) in galaxies. The observation of starburst systems ...
Gas molecular en la nebulosa anillo alrededor de WR 16
(Asociacion Argentina de Astronomía, 2009-01)
Using NANTEN 12CO (J=1→ 0) observations, the distribution of the molecular gas towards the multiple ring nebula sorrounding the star WR 16 has been analysed. Two striking features associated with the star and the nebula, ...
Molecular gas towards G18.8+1.8
(Edp Sciences, 2012-04)
Aims. This work aims at investigating the characteristics of the molecular gas associated with the nebula G18.8+1.8, which is linked to the Wolf-Rayet star HD 168206 (WR 113), and its relation to other components of its ...
Carbon monoxide in clouds at low metallicity in the dwarf irregular galaxy WLM
(Nature Publishing Group, 2013-03-28)
Carbon monoxide (CO) is the primary tracer for interstellar clouds where stars form, but it has never been detected in galaxies in which the oxygen abundance relative to hydrogen is less than 20 per cent of that of the ...
Sh2-206: medio interestelar y formación estelar
(Asociación Argentina de Astronomía, 2009-01)
The analysis of the interstellar matter around the HII region Sh2-206 shows extended emission in a region of more than 30 pc from the optical nebula detected both in the radio continuum and in the far IR. The distribution ...
A model for the onset of self-gravitation and star formation in molecular gas governed by galactic forces. II. The bottleneck to collapse set by cloud-environment decoupling
(IOP Publishing, 2020)
In Meidt et al., we showed that gas kinematics on the scale of individual molecular clouds are not entirely dominated by self-gravity but also track a component that originates with orbital motion in the potential of the ...
Carbon monoxide in the environs of the star WR16
(EDP Sciences, 2013-03)
Aims. We analyze the carbon monoxide emission around the star WR 16 aiming to study the physical characteristics of the molecular gas linked to the star and to achieve a better understanding of the interaction between ...
A submillimeter study of the IR dust bubble S 21 and its environs
(Universidad Nacional Autónoma de México, 2017-04)
Based on the molecular emission in the 12CO(2-1) and 13CO(2-1) lines, and on the continuum emission in the MIR and FIR towards the S 21 IR dust bubble, we analyze the physical characteristics of the gas and dust linked to ...