activity
19992026
most citedFrom filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey

1.5k citations · 11.9k across the 119 of their papers we have counts for

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Showing 2014Show all

12 papers · 1 filter

astro-ph.SR2014★ 29 cited

The JCMT Gould Belt Survey: Evidence for radiative heating in Serpens MWC 297 and its influence on local star formation

D. Rumble, J. Hatchell, R. A. Gutermuth +61

We present SCUBA-2 450micron and 850micron observations of the Serpens MWC 297 region, part of the JCMT Gould Belt Survey of nearby star-forming regions. Simulations suggest that r…

astro-ph.GA2014★ 54 cited

The JCMT Legacy Survey of the Gould Belt: a molecular line study of the Ophiuchus molecular cloud

Glenn J. White, Emily Drabek-Maunder, Erik Rosolowsky +17

CO, CO and CO = 3--2 observations are presented of the Ophiuchus molecular cloud. The CO and CO emission is dominated by the Oph A clump, and…

astro-ph.SR2014★ 57 cited

Revealing H2D+ depletion and compact structure in starless and protostellar cores with ALMA

R. K. Friesen, J. Di Francesco, T. L. Bourke +4

We present Atacama Large Millimeter/submillimeter Array (ALMA) observations of the submillimeter dust continuum and H2D+ 1_{10}-1_{11} emission toward two evolved, potentially prot…

astro-ph.SR2014★ 46 cited

ALMA observations of a misaligned binary protoplanetary disk system in Orion

Jonathan P. Williams, Rita K. Mann, James Di Francesco +6

We present ALMA observations of a wide binary system in Orion, with projected separation 440 AU, in which we detect submillimeter emission from the protoplanetary disks around each…

astro-ph.GA2014★ 24 cited

Signatures of warm carbon monoxide in protoplanetary discs observed with Herschel SPIRE

M. H. D. van der Wiel, D. A. Naylor, I. Kamp +9

Molecular gas constitutes the dominant mass component of protoplanetary discs. To date, these sources have not been studied comprehensively at the longest far-infrared and shortest…

astro-ph.GA2014★ 52 cited

Evidence for Large Grains in the Star-forming Filament OMC-2/3

Scott Schnee, Brian Mason, James Di Francesco +4

We present a new 3.3 mm continuum map of the OMC-2/3 region. When paired with previously published maps of 1.2mm continuum and NH3-derived temperature, we derive the emissivity spe…

astro-ph.SR2014★ 8 cited

The disk around the brown dwarf KPNO Tau 3

Hannah Broekhoven-Fiene, Brenda Matthews, Gaspard Duchene +4

We present submillimeter observations of the young brown dwarfs KPNO Tau 1, KPNO Tau 3, and KPNO Tau 6 at 450 micron and 850 micron taken with the Submillimeter Common-User Bolomet…

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,…

astro-ph.SR2014★ 136 cited

ALMA Observations of the Orion Proplyds

Rita K. Mann, James Di Francesco, Doug Johnstone +6

We present ALMA observations of protoplanetary disks ("proplyds") in the Orion Nebula Cluster. We imaged 5 individual fields at 856um containing 22 HST-identified proplyds and dete…

astro-ph.GA2014★ 101 cited

Fragmentation of massive dense cores down to ~1000 AU: Relation between fragmentation and density structure

Aina Palau, R. Estalella, J. M. Girart +10

In order to shed light on the main physical processes controlling fragmentation of massive dense cores, we present a uniform study of the density structure of 19 massive dense core…

astro-ph.GA2014★ 46 cited

Properties of Starless and Prestellar Cores in Taurus Revealed by Herschel SPIRE/PACS Imaging

K. A. Marsh, M. J. Griffin, P. Palmeirim +18

The density and temperature structures of dense cores in the L1495 cloud of the Taurus star-forming region are investigated using Herschel SPIRE and PACS images in the 70 m, 160…

astro-ph.GA2014★ 97 cited

Ionization compression impact on dense gas distribution and star formation, Probability density functions around H ii regions as seen by Herschel

P. Tremblin, N. Schneider, V. Minier +22

Ionization feedback should impact the probability distribution function (PDF) of the column density around the ionized gas. We aim to quantify this effect and discuss its potential…