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Are the host galaxies of Long Gamma-Ray Bursts more compact than star-forming galaxies of the field?

Are the host galaxies of Long Gamma-Ray Bursts more compact than star-forming galaxies of the field?

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2682963423

Are the host galaxies of Long Gamma-Ray Bursts more compact than star-forming galaxies of the field?

About this item

Full title

Are the host galaxies of Long Gamma-Ray Bursts more compact than star-forming galaxies of the field?

Publisher

Ithaca: Cornell University Library, arXiv.org

Journal title

arXiv.org, 2022-06

Language

English

Formats

Publication information

Publisher

Ithaca: Cornell University Library, arXiv.org

More information

Scope and Contents

Contents

(Abridged) Long Gamma-Ray Bursts (GRBs) offer a promising tool to trace the cosmic history of star formation, especially at high redshift where conventional methods are known to suffer from intrinsic biases. Previous studies of GRB host galaxies at low redshift showed that high surface densities of stellar mass and star formation rate (SFR) can pot...

Alternative Titles

Full title

Are the host galaxies of Long Gamma-Ray Bursts more compact than star-forming galaxies of the field?

Authors, Artists and Contributors

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_2682963423

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2682963423

Other Identifiers

E-ISSN

2331-8422

DOI

10.48550/arxiv.2206.14873

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