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Massive-Star Feedback at Low Metallicity

Published online by Cambridge University Press:  13 February 2024

M. S. Oey Open the ORCID record for M. S. Oey [Opens in a new window] ,
M. C. Jecmen ,
A. N. Sawant ,
A. E. Jaskot Open the ORCID record for A. E. Jaskot [Opens in a new window] ,
A. Danehkar ,
L. J. Smith  and
J. Melinder
M. S. Oey*
Affiliation:
University of Michigan, Department of Astronomy, Ann Arbor, MI, 48109, USA
M. C. Jecmen
Affiliation:
University of Michigan, Department of Astronomy, Ann Arbor, MI, 48109, USA
A. N. Sawant
Affiliation:
University of Michigan, Department of Astronomy, Ann Arbor, MI, 48109, USA Current address: EPFL, Institute of Mathematics, MA C2 647, Station 8, CH-1015 Lausanne, Switzerland
A. E. Jaskot
Affiliation:
Williams College, Department of Astronomy, Williamstown, MA 01267, USA
A. Danehkar
Affiliation:
Current address: Eureka Scientific, 2452 Delmer St., Suite 100, Oakland, CA 94602, USA
L. J. Smith
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA
J. Melinder
Affiliation:
Stockholm University, Department of Astronomy, Oscar Klein Centre, AlbaNova University Centre, SE-10691 Stockholm, Sweden
*
email: [email protected]
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Abstract

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Early cosmic epochs are characterized by low metallicity and high specific star-formation rates. These conditions are dominated by massive-star feedback that may be dramatically different than the traditional model dominated by hot, thermal superwinds driven by supernova explosions. Instead, metal-poor feedback from massive stars may be radiation-dominated, with weak mechanical feedback, possibly aiding the escape of Lyα and Lyman continuum radiation. I will describe our understanding that is emerging from observations of starburst galaxies in the local universe.

Keywords

massive starsgalactic windssuperbubblesyoung massive clusterscore-collapse supernovaestarburst galaxiesemission-line galaxiesgalaxy evolutionreionization
Type
Contributed Paper
Information
Proceedings of the International Astronomical Union , Volume 18 , Symposium S377: Early Disk-Galaxy Formation from JWST to the Milky Way , December 2022 , pp. 14 - 21
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Creative Commons
Creative Common License - CCCreative Common License - BY
This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted re-use, distribution and reproduction, provided the original article is properly cited.
Copyright
© The Author(s), 2024. Published by Cambridge University Press on behalf of International Astronomical Union

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