The link between star formation and gas in nearby galaxies

How galaxies form their stars has been extensively studied but the role of the galactic gas content and the efficiency of its conversion into stars remain to be fully understood. Here the author presents a data-driven statistical analysis that reduces potential biases related to non-detections to qu...

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Main Author: Robert Feldmann
Format: Article
Language:English
Published: Nature Publishing Group 2020-12-01
Series:Communications Physics
Online Access:https://doi.org/10.1038/s42005-020-00493-0
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spelling doaj-6c7d8f2eb031423c878472324fc0b5322020-12-07T23:18:06ZengNature Publishing GroupCommunications Physics2399-36502020-12-013111010.1038/s42005-020-00493-0The link between star formation and gas in nearby galaxiesRobert Feldmann0Institute for Computational Science, University of ZurichHow galaxies form their stars has been extensively studied but the role of the galactic gas content and the efficiency of its conversion into stars remain to be fully understood. Here the author presents a data-driven statistical analysis that reduces potential biases related to non-detections to quantify the link between star formation, molecular, and neutral gas in nearby galaxies.https://doi.org/10.1038/s42005-020-00493-0
collection DOAJ
language English
format Article
sources DOAJ
author Robert Feldmann
spellingShingle Robert Feldmann
The link between star formation and gas in nearby galaxies
Communications Physics
author_facet Robert Feldmann
author_sort Robert Feldmann
title The link between star formation and gas in nearby galaxies
title_short The link between star formation and gas in nearby galaxies
title_full The link between star formation and gas in nearby galaxies
title_fullStr The link between star formation and gas in nearby galaxies
title_full_unstemmed The link between star formation and gas in nearby galaxies
title_sort link between star formation and gas in nearby galaxies
publisher Nature Publishing Group
series Communications Physics
issn 2399-3650
publishDate 2020-12-01
description How galaxies form their stars has been extensively studied but the role of the galactic gas content and the efficiency of its conversion into stars remain to be fully understood. Here the author presents a data-driven statistical analysis that reduces potential biases related to non-detections to quantify the link between star formation, molecular, and neutral gas in nearby galaxies.
url https://doi.org/10.1038/s42005-020-00493-0
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