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19992025
most citedFrom filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey

1.5k citations · 9.9k across the 91 of their papers we have counts for

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astro-ph.SR2019★ 122 cited

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…

astro-ph.SR2016★ 34 cited

Remarkable analytic relations among greybody parameters

Davide Elia, Stefano Pezzuto

In this paper we derive and discuss several implications of the analytic form of a modified blackbody, also called greybody, which is widely used in Astrophysics, and in particular…

astro-ph.SR2015★ 28 cited

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…

astro-ph.SR2015★ 5 cited

The Kinematic and Chemical Properties of a Potential Core-Forming Clump: Perseus B1-E

Sarah I. Sadavoy, Yancy Shirley, James Di Francesco +4

We present 13CO and C18O (1-0), (2-1), and (3-2) maps towards the core-forming Perseus B1-E clump using observations from the James Clerk Maxwell Telescope (JCMT), Submillimeter Te…

astro-ph.SR2014★ 11 cited

The YSO Population in the Vela-D Molecular Cloud

F. Strafella, D. Lorenzetti, T. Giannini +7

We investigate the young stellar population in the Vela Molecular Ridge, Cloud-D (VMR-D), a star forming (SF) region observed by both Spitzer/NASA and Herschel/ESA space telescope.…

astro-ph.SR2014★ 119 cited

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,…