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  Molecular Line Emission as a Tool for Galaxy Observations (LEGO). I. HCN as a tracer of moderate gas densities in molecular clouds and galaxies

Kauffmann, J., Goldsmith, P., Melnick, G., Tolls, V., Guzman, A., & Menten, K. (2017). Molecular Line Emission as a Tool for Galaxy Observations (LEGO). I. HCN as a tracer of moderate gas densities in molecular clouds and galaxies. Astronomy and Astrophysics, 605: L5, pp. L5. doi:10.1051/0004-6361/201731123.

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Kauffmann, J.1, Author
Goldsmith, P.F., Author
Melnick, G., Author
Tolls, V., Author
Guzman, A., Author
Menten, K.M.1, Author
Affiliations:
1Max Planck Institute for Radio Astronomy, Max Planck Society, ou_2205652              

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Free keywords: stars: formation, ISM: clouds, ISM: molecules, galaxies: evolution, galaxies: ISM, galaxies: star formation
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 Dates: 2017-09
 Publication Status: Issued
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 Rev. Type: -
 Identifiers: DOI: 10.1051/0004-6361/201731123
BibTex Citekey: 2017a&a...605l...5k
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Title: Astronomy and Astrophysics
Source Genre: Journal
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Pages: - Volume / Issue: 605 Sequence Number: L5 Start / End Page: L5 Identifier: -