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Ragan, S. E.
Ragan, Sarah E.
Ragan, S.
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http://hub.abes.fr/edp/periodical/aa/2012/volume_547/issue_2012/aa19232-12/authorship/1
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The HI/OH/Recombination line survey of the inner Milky Way (THOR)
Are infrared dark clouds really quiescent?
The seeds of star formation in the filamentary infrared-dark cloud G011.11-0.12
Filament fragmentation in high-mass star formation
High-fidelity view of the structure and fragmentation of the high-mass, filamentary IRDC G11.11-0.12
Giant molecular filaments in the Milky Way
The onset of high-mass star formation in the direct vicinity of the Galactic mini-starburst W43
The Earliest Phases of Star Formation (EPoS): a Herschel key program
The Earliest Phases of Star Formation (EPoS): a Herschel key project
Giant molecular filaments in the Milky Way
The Earliest Phases of Star formation (EPoS) observed with Herschel: the dust temperature and density distributions of B68
Carbon in different phases ([CII], [CI], and CO) in infrared dark clouds: Cloud formation signatures and carbon gas fractions
THOR: The H i, OH, Recombination line survey of the Milky Way
Earliest phases of star formation (EPoS)
Fragmentation and dynamical collapse of the starless high-mass star-forming region IRDC 18310-4
APEX/SABOCA observations of small-scale structure of infrared-dark clouds
Kinematic structure of massive star-forming regions
The dynamics and star-forming potential of the massive Galactic centre cloud G0.253+0.016
Fragmentation and kinematics of dense molecular cores in the filamentary infrared-dark cloud G011.11-0.12
Carbon in different phases ([CII], [CI], and CO) in infrared dark clouds: Cloud formation signatures and carbon gas fractions (Corrigendum)
Kinematic and thermal structure at the onset of high-mass star formation
Hierarchical fragmentation and collapse signatures in a high-mass starless region
Fragmentation and disk formation during high-mass star formation
OH absorption in the first quadrant of the Milky Way as seen by THOR
Core fragmentation and Toomre stability analysis of W3(H 2O)
Feedback in W49A diagnosed with radio recombination lines and models
Histogram of oriented gradients: a technique for the study of molecular cloud formation
CHIMPS: physical properties of molecular clumps across the inner Galaxy
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