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From global to local scales in galaxies

Published online by Cambridge University Press:  29 March 2021

Sebastian F. Sánchez Open the ORCID record for Sebastian F. Sánchez [Opens in a new window]  and
Carlos Lopez Cobá
Sebastian F. Sánchez
Affiliation:
Instituto de Astronomía, Universidad Nacional Autonóma de México, A.P. 70-264, 04510 México, D.F., Mexico email: sfsanchez@astro.unam.mx
Carlos Lopez Cobá
Affiliation:
Instituto de Astronomía, Universidad Nacional Autonóma de México, A.P. 70-264, 04510 México, D.F., Mexico email: sfsanchez@astro.unam.mx
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Abstract

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We summarize here some of the results reviewed recently by Sanchez (2020) comprising the advances in the comprehension of galaxies in the nearby universe based on integral field spectroscopic galaxy surveys. In particular we explore the bimodal distribution of galaxies in terms of the properties of their ionized gas, showing the connection between the star-formation (quenching) process with the presence (absence) of molecular gas and the star-formation efficiency. We show two galaxy examples that illustrates the well known fact that ionization in galaxies (and the processes that produce it), does not happen monolitically at galactic scales. This highlight the importance to explore the spectroscopic properties of galaxies and the evolutionary processes unveiled by them at different spatial scales, from sub-kpc to galaxy wide.

Keywords

galaxies: evolutiongalaxies: star-formationgalaxies: ISM
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 15 , Symposium S359: Galaxy Evolution and Feedback across Different Environments , March 2019 , pp. 391 - 395
Copyright
© The Author(s), 2021. Published by Cambridge University Press on behalf of International Astronomical Union

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