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  Imaging molecular gas in high redshift galaxies at <=1 kpc resolution

Carilli, C., Casey, C., Narayanan, D., Bolatto, A., Hung, C., Champagne, J., et al. (2019). Imaging molecular gas in high redshift galaxies at <=1 kpc resolution. Bulletin of the American Astronomical Society, 51.

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Item Permalink: https://hdl.handle.net/21.11116/0000-0005-D1A4-5 Version Permalink: https://hdl.handle.net/21.11116/0000-0005-D1A5-4
Genre: Journal Article

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https://ui.adsabs.harvard.edu/abs/2019BAAS...51c..41C (Any fulltext)
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 Creators:
Carilli, Christopher1, Author
Casey, C.1, Author
Narayanan, D.1, Author
Bolatto, A.1, Author
Hung, C.1, Author
Champagne, J.1, Author
Walter, F.1, Author
Riechers, D.1, Author
Murphy, E.1, Author
Decarli, R.1, Author
Affiliations:
1Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners, ou_2421692              

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 Abstract: Imaging the cool molecular gas in distant galaxies, the fuel for star formation, at &lt;= 1 kpc resolution, is a prerequisite for future 'precision galaxy formation studies', addressing such basic issues as a Universal 'star formation law', cloud evolution and feed-back, and the dynamics and physical conditions in the cold gas in early galaxies.

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 Dates: 2019
 Publication Status: Issued
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Title: Bulletin of the American Astronomical Society
Source Genre: Journal
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Pages: - Volume / Issue: 51 Sequence Number: - Start / End Page: - Identifier: -