activity
20022024
most citedWhat determines the density structure of molecular clouds ? A case study of Orion B with Herschel

270 citations · 762 across the 12 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2024

A study of Galactic Plane Planck Galactic Cold Clumps observed by SCOPE and the JCMT Plane Survey

D. J. Eden, Tie Liu, T. J. T. Moore +32

We have investigated the physical properties of Planck Galactic Cold Clumps (PGCCs) located in the Galactic Plane, using the JCMT Plane Survey (JPS) and the SCUBA-2 Continuum Obser…

astro-ph.GA2020★ 48 cited

Physical properties of the ambient medium and of dense cores in the Perseus star-forming region derived from Herschel Gould Belt Survey observations

S. Pezzuto, M. Benedettini, J. Di Francesco +20

(Abridged) In this paper, we present analyses of images taken with the Herschel ESA satellite from 70mu to 500mu. We first constructed column density and dust temperature maps. Nex…

astro-ph.GA2018★ 55 cited

A catalogue of dense cores and young stellar objects in the Lupus complex based on Herschel Gould Belt Survey observations

M. Benedettini, S. Pezzuto, E. Schisano +13

The Herschel Gould Belt Survey key project mapped the bulk of nearby star-forming molecular clouds in five far-infrared bands with the aim of compiling complete census of prestella…

astro-ph.SR2016★ 42 cited

Herschel detects oxygen in the beta Pictoris debris disk

A. Brandeker, G. Cataldi, G. Olofsson +28

The young star beta Pictoris is well known for its dusty debris disk, produced through the grinding down by collisions of planetesimals, kilometre-sized bodies in orbit around the…

astro-ph.GA2016★ 19 cited

Globules and Pillars in Cygnus X I. Herschel Far-infrared imaging of the Cyg OB2 environment

N. Schneider, S. Bontemps, F. Motte +21

The radiative feedback of massive stars on molecular clouds creates pillars, globules and other features at the interface between the HII region and molecular cloud. We present her…

astro-ph.GA2016★ 43 cited

Dust Emissivity in the Star-Forming Filament OMC 2/3

S. I. Sadavoy, A. M. Stutz, S. Schnee +3

We present new measurements of the dust emissivity index, beta, for the high-mass, star-forming OMC 2/3 filament. We combine 160-500 um data from Herschel with long-wavelength obse…