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Battersby, Cara
Battersby, C.
Battersby, C. D.
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cara.battersby@colorado.edu
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Cara
C. D.
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http://hub.abes.fr/edp/periodical/aa/2016/volume_586/issue_2016/aa26100-15/authorship/13
http://hub.abes.fr/edp/periodical/aa/2010/volume_518/issue_2010/aa14651-10/authorship/7
http://hub.abes.fr/edp/periodical/aa/2010/volume_518/issue_2010/aa14659-10/authorship/17
http://hub.abes.fr/edp/periodical/aa/2011/volume_526/issue_2011/aa15488-10/authorship/6
http://hub.abes.fr/edp/periodical/aa/2011/volume_535/issue_2011/aa16559-11/authorship/1
http://hub.abes.fr/edp/periodical/eas/2016/volume_7576/issue_2016/eas1575006/authorship/6
http://hub.abes.fr/edp/periodical/aa/2010/volume_518/issue_2010/aa14596-10/authorship/3
http://hub.abes.fr/edp/periodical/aa/2016/volume_595/issue_2016/aa28318-16/authorship/7
http://hub.abes.fr/edp/periodical/aa/2020/volume_641/issue_2020/aa37928-20/authorship/8
http://hub.abes.fr/edp/periodical/aa/2015/volume_584/issue_2015/aa27452-15/authorship/12
http://hub.abes.fr/edp/periodical/aa/2010/volume_518/issue_2010/aa14652-10/authorship/6
http://hub.abes.fr/edp/periodical/aa/2015/volume_573/issue_2015/aa24979-14/authorship/3
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of
The dense gas mass fraction in the W51 cloud and its protoclusters
Dense gas in the Galactic central molecular zone is warm and heated by turbulence
Toward gas exhaustion in the W51 high-mass protoclusters
Using young massive star clusters to understand star formation and feedback in high-redshift-like environments
The initial conditions of high-mass star formation: radiative transfer models of IRDCs seen in the Herschel Hi-GAL survey
Dense gas in a giant molecular filament
Clouds, filaments, and protostars: The Herschel Hi-GAL Milky Way
Characterizing precursors to stellar clusters with Herschel
High-mass star-forming cloud G0.38+0.04 in the Galactic center dust ridge contains H 2CO and SiO masers
Herschel observations of the W43 “mini-starburst”
A Herschel study of YSO evolutionary stages and formation timelines in two fields of the Hi-GAL survey
Mapping the column density and dust temperature structure of IRDCs with Herschel
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