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Star formation traced by optical and millimeter hydrogen recombination lines and free-free emissions...

Star formation traced by optical and millimeter hydrogen recombination lines and free-free emissions...

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2389948382

Star formation traced by optical and millimeter hydrogen recombination lines and free-free emissions in the dusty merging galaxy NGC 3256 -- MUSE/VLT and ALMA synergy

About this item

Full title

Star formation traced by optical and millimeter hydrogen recombination lines and free-free emissions in the dusty merging galaxy NGC 3256 -- MUSE/VLT and ALMA synergy

Publisher

Ithaca: Cornell University Library, arXiv.org

Journal title

arXiv.org, 2020-04

Language

English

Formats

Publication information

Publisher

Ithaca: Cornell University Library, arXiv.org

More information

Scope and Contents

Contents

A galaxy-galaxy merger and the subsequent triggering of starburst activity are fundamental processes linked to the morphological transformation of galaxies and the evolution of star formation across the history of the Universe. Both nuclear and disk-wide starbursts are assumed to occur during the merger process. However, quantifying both nuclear an...

Alternative Titles

Full title

Star formation traced by optical and millimeter hydrogen recombination lines and free-free emissions in the dusty merging galaxy NGC 3256 -- MUSE/VLT and ALMA synergy

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_2389948382

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2389948382

Other Identifiers

E-ISSN

2331-8422

DOI

10.48550/arxiv.2004.06123

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