G11.92–0.61-MM2: A BONAFIDE MASSIVE PRESTELLAR CORE?-Reference-Cited by-同舟云学术

G11.92–0.61-MM2: A BONAFIDE MASSIVE PRESTELLAR CORE?

Published:2014-10-31 Issue:1 Volume:796 Page:L2
ISSN:2041-8213
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Cyganowski C. J.^ORCID,Brogan C. L.^ORCID,Hunter T. R.^ORCID,Graninger D.^ORCID,Öberg K. I.^ORCID,Vasyunin A.,Zhang Q.^ORCID,Friesen R.^ORCID,Schnee S.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.1088/2041-8205/796/1/L2/pdf

Reference46 articles.

1. The mass function of dense molecular cores and the origin of the IMF

2. Chemical Evolution in Preprotostellar and Protostellar Cores

3. Fragmentation and mass segregation in the massive dense cores of Cygnus X

4. Constraining the properties of 1.2-mm dust clumps that contain luminous water masers

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