Filamentary structure and Keplerian rotation in the high-mass star-forming region G35.03+0.35 imaged with ALMA-Reference-Cited by-同舟云学术

Filamentary structure and Keplerian rotation in the high-mass star-forming region G35.03+0.35 imaged with ALMA

Published:2014-11 Issue: Volume:571 Page:A52
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Beltrán M. T.,Sánchez-Monge Á.,Cesaroni R.,Kumar M. S. N.,Galli D.,Walmsley C. M.,Etoka S.,Furuya R. S.,Moscadelli L.,Stanke T.,van der Tak F. F. S.,Vig S.,Wang K.-S.,Zinnecker H.,Elia D.,Schisano E.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361/201424031/pdf

Reference78 articles.

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3. Beltrán, M. T. 2011, in Computational Star Formation, eds. J. Alves, B. G. Elmegreen, J. M. Girart et al., Proc. IAU Symp., 270, 33

4. A detailed study of the rotating toroids in G31.41+0.31 and G24.78+0.08

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