Dust and gas in star-forming complexes in NGC 3351, NGC 5055, and NGC 5457-Reference-Cited by-同舟云学术

Dust and gas in star-forming complexes in NGC 3351, NGC 5055, and NGC 5457

Published:2023-01-01 Issue:1 Volume:32 Page:
ISSN:2543-6376
Container-title:Open Astronomy
language:en
Short-container-title:

Author:

Smirnova Ksenia Ildarovna¹,Wiebe Dmitri Siegfriedovich²

Affiliation:

1. Institute of Natural Sciences and Mathematics, Ural Federal University , Ekaterinburg , 620002 , Russian Federation

2. Institute of Astronomy, Russian Academy of Sciences , Moscow , Russian Federation

Abstract

Abstract We present a study of the interstellar medium parameters in star-forming complexes (SFCs) in NGC 3351, NGC 5055, and NGC 5457 galaxies. This study concludes our previous investigations of gas and dust in a number of spiral galaxies. The data for the three galaxies confirm the following. There is a tight correlation between near-infrared and far-infrared luminosities of the extragalactic SFCs. Emission at 8 μm also shows a strong correlation with the carbon monoxide emission. Atomic and molecular gas masses do not show any strong correlation with the corresponding velocity scatters; however, in NGC 5055, we see a hint of the SFC with the largest velocity scatter being located at the galaxy periphery.

Publisher

Walter de Gruyter GmbH

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://www.degruyter.com/document/doi/10.1515/astro-2022-0219/pdf

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