The Seven Most Massive Clumps in W43-Main as Seen by ALMA: Dynamical Equilibrium and Magnetic Fields-Reference-Cited by-同舟云学术

The Seven Most Massive Clumps in W43-Main as Seen by ALMA: Dynamical Equilibrium and Magnetic Fields

Published:2019-10-11 Issue:1 Volume:884 Page:48
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Cortes Paulo C.^ORCID,Hull Charles L. H.^ORCID,Girart Josep M.^ORCID,Orquera-Rojas Carlos,Sridharan Tirupati K.,Li Zhi-Yun,Louvet Fabien,Cortes Juan R.,Le Gouellec Valentin J. M.,Crutcher Richard M.,Lai Shih-Ping^ORCID

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/1538-4357/ab378d/pdf

Reference86 articles.

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

2. Characterizing filaments in regions of high-mass star formation: High-resolution submilimeter imaging of the massive star-forming complex NGC 6334 with ArTéMiS

3. Characterizing interstellar filaments withHerschelin IC 5146

4. Herschelobservations of the W43 “mini-starburst”

5. VLA High-Sensitivity [TSUP]4[/TSUP]H[CLC]e[/CLC] Imaging of Galactic H [CSC]ii[/CSC] Regions

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