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The local and global relations between Σ*, ΣSFR and Σmol that regulate star-formation

Published online by Cambridge University Press:  09 June 2023

Sebastián F. Sánchez Open the ORCID record for Sebastián F. Sánchez [Opens in a new window] ,
Daysi C. Gómez Medina ,
J.K. Barrera-Ballesteros ,
L. Galbany ,
A. Bolatto Open the ORCID record for A. Bolatto [Opens in a new window]  and
T. Wong Open the ORCID record for T. Wong [Opens in a new window]
Sebastián F. Sánchez
Affiliation:
Instituto de Astronomía, Universidad Nacional Autónoma de México, A. P. 70-264, C.P. 04510, Ciudad de México, Mexico Email: [email protected]
Daysi C. Gómez Medina
Affiliation:
Facultad de Ciencias Espaciales, Universidad Nacional Autónoma de Honduras
J.K. Barrera-Ballesteros
Affiliation:
Instituto de Astronomía, Universidad Nacional Autónoma de México, A. P. 70-264, C.P. 04510, Ciudad de México, Mexico Email: [email protected]
L. Galbany
Affiliation:
Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans, s/n, E-08193 Barcelona, Spain.
A. Bolatto
Affiliation:
Department of Astronomy, University of Maryland, College Park, MD 20742, USA
T. Wong
Affiliation:
Department of Astronomy, University of Illinois, Urbana, IL 61801, USA
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Abstract

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Star-formation is one of the main processes that shape galaxies, defining its stellar population and metallicity production and enrichment. It is nowadays known that this process is ruled by a set of relations that connect three parameters: the molecular gas mass, the stellar mass and the star-formation rate itself. These relations are fulfilled at a wide range of scales in galaxies, from galaxy wide to kpc-scales. At which scales they are broken, and how universal they are (i.e., if they change at different scales or for different galaxy types) it is still an open question. We explore here how those relations compare at different scales using as proxy the new analysis done using Integral Field Spectroscopy data and CO observations data from the EDGE-CALIFA survey and the AMUSSING++ compilation.

Keywords

galaxies: evolutiongalaxies: ISMgalaxies: TBWtechniques: spectroscopic
Type
Contributed Paper
Information
Proceedings of the International Astronomical Union , Volume 17 , Symposium S373: Resolving the Rise and Fall of Star Formation in Galaxies , August 2021 , pp. 3 - 10
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Copyright
© The Author(s), 2023. Published by Cambridge University Press on behalf of International Astronomical Union

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