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Anatomy of Galactic Star Formation: Roles of Different Modes of Gas Accretion, Feedback, and Recycling

Published online by Cambridge University Press:  09 June 2023

Masafumi Noguchi Open the ORCID record for Masafumi Noguchi [Opens in a new window]
Masafumi Noguchi*
Affiliation:
Astronomical Institute, Tohoku University, 6-3, Aramaki, Aoba-ku, Sendai, Miyagi, 980-8578, Japan email: noguchi@astr.tohoku.ac.jp
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Abstract

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Existence of the cold-mode gas accretion along with the hot-mode accretion can explain the diversity in the galactic star formation history across galaxy mass. We examine the role of various physical processes in producing the observed diversity.

Keywords

galaxies: evolutiongalaxies: high-redshiftgalaxies: starburst
Type
Poster Paper
Information
Proceedings of the International Astronomical Union , Volume 17 , Symposium S373: Resolving the Rise and Fall of Star Formation in Galaxies (Aug 2022) , August 2021 , pp. 325 - 327
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Copyright
© The Author(s), 2023. Published by Cambridge University Press on behalf of International Astronomical Union

References

Behroozi, P. et al. 2019, Mon. Not. Roy. Astr. Soc., 488, 3143 10.1093/mnras/stz1182CrossRefGoogle Scholar
Moster, B.P., Naab, T., & White, S.D.M. 2013, Mon. Not. Roy. Astr. Soc., 428, 3121 10.1093/mnras/sts261CrossRefGoogle Scholar
Noguchi, M. 2022, submitted to Mon. Not. Roy. Astr. Soc. Google Scholar
Whitaker, K.E. et al. 2014, ApJ, 795, 10410.1088/0004-637X/795/2/104CrossRefGoogle Scholar