activity
20002018
most citedClouds, filaments and protostars: the Herschel Hi-GAL Milky Way

806 citations · 3.4k across the 27 of their papers we have counts for

collaborators

23 papers

astro-ph.HE2018★ 29 cited

Radio observations of the double-relic galaxy cluster Abell 1240

D. N. Hoang, T. W. Shimwell, R. J. van Weeren +16

We present LOFAR MHz images of the merging galaxy cluster Abell 1240 that hosts double radio relics. In combination with the GMRT MHz and VLA GHz data, we…

astro-ph.GA2017★ 95 cited

The earliest phases of high-mass star formation, as seen in NGC 6334 by \emph{Herschel}

J. Tigé, F. Motte, D. Russeil +33

To constrain models of high-mass star formation, the Herschel/HOBYS KP aims at discovering massive dense cores (MDCs) able to host the high-mass analogs of low-mass prestellar core…

astro-ph.GA2015★ 28 cited

The JCMT Gould Belt Survey: SCUBA-2 observations of circumstellar disks in L 1495

J. V. Buckle, E. Drabek-Maunder, J. Greaves +51

We present 850m and 450m data from the JCMT Gould Belt Survey obtained with SCUBA-2 and characterise the dust attributes of Class I, Class II and Class III disk sources in L1…

astro-ph.GA2013★ 51 cited

Herschel Observations of the W3 GMC: Clues to the Formation of Clusters of High-Mass Stars

A. Rivera-Ingraham, P. G. Martin, D. Polychroni +22

The W3 GMC is a prime target for the study of the early stages of high-mass star formation. We have used Herschel data from the HOBYS key program to produce and analyze column dens…

astro-ph.SR2012★ 31 cited

Centauri A in the far infrared

R. Liseau, B. Montesinos, G. Olofsson +15

Chromospheres and coronae are common phenomena on solar-type stars. Understanding the energy transfer to these heated atmospheric layers requires direct access to the relevant empi…

astro-ph.SR2012★ 595 cited

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…