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  ATLASGAL - physical parameters of dust clumps associated with 6.7 GHz methanol masers

Billington, S., Urquhart, J., König, C., Moore, T., Eden, D., Breen, S., et al. (2019). ATLASGAL - physical parameters of dust clumps associated with 6.7 GHz methanol masers. mnras, 490(2), 2779-2798. doi:10.1093/mnras/stz2691.

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 Creators:
Billington, S.J., Author
Urquhart, J.S., Author
König, C.1, Author
Moore, T.J.T., Author
Eden, D.J., Author
Breen, S.L., Author
Kim, W.-J., Author
Thompson, M.A., Author
Ellingsen, S.P., Author
Menten, K.M.1, Author
Wyrowski, F.1, Author
Leurini, S.1, Author
Affiliations:
1Max Planck Institute for Radio Astronomy, Max Planck Society, ou_2205652              

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Free keywords: stars: formation, stars: massive, ISM: molecules, submillimetre: ISM, Astrophysics - Astrophysics of Galaxies
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 Dates: 2019-12
 Publication Status: Issued
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: -
 Identifiers: DOI: 10.1093/mnras/stz2691
BibTex Citekey: 2019MNRAS.490.2779B
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Title: mnras
Source Genre: Journal
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Publ. Info: -
Pages: - Volume / Issue: 490 (2) Sequence Number: - Start / End Page: 2779 - 2798 Identifier: -