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Filamentary Network and Magnetic Field Structures Revealed with BISTRO in the High-Mass Star-Forming Region NGC2264 : Global Properties and Local Magnetogravitational Configurations
Jia-Wei Wang, Patrick M. Koch, Seamus D. Clarke +154
We report 850 m continuum polarization observations toward the filamentary high-mass star-forming region NGC 2264, taken as part of the B-fields In STar forming Regions Observat…
Properties of the dense core population in Orion B as seen by the Herschel Gould Belt survey
V. Konyves, Ph. Andre, D. Arzoumanian +15
We present a detailed study of the Orion B clouds (d~400 pc), imaged with the PACS/SPIRE cameras at 70-500 m by the Herschel Gould Belt survey (HGBS). We release new high-res. m…
From forced collapse to H ii region expansion in Mon R2: Envelope density structure and age determination with Herschel
P. Didelon, F. Motte, P. Tremblin +32
The surroundings of HII regions can have a profound influence on their development, morphology, and evolution. This paper explores the effect of the environment on H II regions in…
Class 0 Protostars in the Perseus Molecular Cloud: A Correlation Between the Youngest Protostars and the Dense Gas Distribution
S. I. Sadavoy, J. Di Francesco, Ph. Andre +18
We use PACS and SPIRE continuum data at 160 um, 250 um, 350 um, and 500 um from the Herschel Gould Belt Survey to sample seven clumps in Perseus: B1, B1-E, B5, IC348, L1448, L1455,…
Formation and evolution of interstellar filaments; Hints from velocity dispersion measurements
Doris Arzoumanian, Philippe André, Nicolas Peretto +1
We investigate the gas velocity dispersions of a sample of filaments recently detected as part of the Herschel Gould Belt Survey in the IC5146, Aquila, and Polaris interstellar clo…
Herschel view of the Taurus B211/3 filament and striations: Evidence of filamentary growth?
P. Palmeirim, Ph. André, J. Kirk +23
We present first results from the Herschel Gould Belt survey for the B211/L1495 region in the Taurus molecular cloud. Thanks to their high sensitivity and dynamic range, the Hersch…
Resolving the Vela C ridge with P-ArTeMiS and Herschel
T. Hill, Ph. Andre, D. Arzoumanian +25
We present APEX/P-ArTéMiS 450μm continuum observations of RCW 36 and the adjacent ridge, a high-mass high-column density filamentary structure at the centre of the Vela C molecular…
The Aquila prestellar core population revealed by Herschel
V. Könyves, Ph. André, A. Men'shchikov +37
The origin and possible universality of the stellar initial mass function (IMF) is a major issue in astrophysics. One of the main objectives of the Herschel Gould Belt Survey is to…