activity
20062025
most citedClouds, filaments and protostars: the Herschel Hi-GAL Milky Way

806 citations · 7k across the 100 of their papers we have counts for

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Showing 2013Show all

12 papers · 1 filter

astro-ph.GA2013★ 133 cited

Rotationally-supported disks around Class I sources in Taurus: disk formation constraints

Daniel Harsono, Jes K. Jorgensen, Ewine F. van Dishoeck +4

(Abridged) Disks are observed around pre-main sequence stars, but how and when they form is still heavily debated. While disks around young stellar objects have been identified thr…

astro-ph.GA2013★ 171 cited

The RMS Survey: Galactic distribution of massive star formation

J. S. Urquhart, C. C. Figura, T. J. T. +6

Abridged: We have used the well-selected sample of ~1750 embedded, young, massive stars identified by the RMS survey to investigate the Galactic distribution of recent massive star…

astro-ph.GA2013★ 48 cited

Deuterated water in the solar-type protostars NGC 1333 IRAS 4A and IRAS 4B

A. Coutens, C. Vastel, S. Cabrit +19

Aims. The aim of this paper is to study deuterated water in the solar-type protostars NGC1333 IRAS4A and IRAS4B, to compare their HDO abundance distribution with other star-forming…

astro-ph.GA2013★ 289 cited

The Red MSX Source Survey: the Massive Young Stellar Population of our Galaxy

S. L. Lumsden, M. G. Hoare, J. S. Urquhart +5

We present the Red MSX Source (RMS) Survey, the largest statistically selected catalog of young massive protostars and HII regions to date. We outline the construction of the catal…

astro-ph.GA2013★ 42 cited

Waterfalls around protostars: Infall motions towards Class 0/I envelopes as probed by water

J. C. Mottram, E. F. van Dishoeck, M. Schmalzl +4

Abridged abstract: For stars to form, material must fall inwards from core scales through the envelope towards the central protostar. The velocity profile around protostars is poor…

astro-ph.SR2013★ 116 cited

ALMA imaging of the CO snowline of the HD 163296 disk with DCO+

G. S. Mathews, P. D. Klaassen, A. Juhasz +11

The high spatial and line sensitivity of ALMA opens the possibility of resolving emission from molecules in circumstellar disks. With an understanding of physical conditions under…