most citedResolving debris discs in the far-infrared: early highlights from the DEBRIS survey

111 citations · 279 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2010★ 18 cited

HERSCHEL-HIFI spectroscopy of the intermediate mass protostar NGC7129 FIRS 2

D. Johnstone, M. Fich, C. McCoey +58

HERSCHEL-HIFI observations of water from the intermediate mass protostar NGC7129 FIRS 2 provide a powerful diagnostic of the physical conditions in this star formation environment.…

astro-ph.GA2010★ 16 cited

Herschel observations of deuterated water towards Sgr B2(M)

Claudia Comito, Peter Schilke, Rainer Rolffs +53

Observations of HDO are an important complement for studies of water, because they give strong constraints on the formation processes -- grain surfaces versus energetic process in…

astro-ph.GA2010★ 53 cited

Herschel observations of extra-ordinary sources: Detection of Hydrogen Fluoride in absorption towards Orion~KL

T. G. Phillips, E. A. Bergin, D. C. Lis +52

We report a detection of the fundamental rotational transition of hydrogen fluoride in absorption towards Orion KL using Herschel/HIFI. After the removal of contaminating features…

astro-ph.GA2010★ 30 cited

Herschel-PACS spectroscopy of the intermediate mass protostar NGC7129 FIRS 2

M. Fich, D. Johnstone, T. A. van Kempen +58

Aims: We present preliminary results of the first Herschel spectroscopic observations of NGC7129 FIRS2, an intermediate mass star-forming region. We attempt to interpret the observ…

astro-ph.SR2010★ 111 cited

Resolving debris discs in the far-infrared: early highlights from the DEBRIS survey

DEBRIS Collaboration, Brenda Matthews, Bruce Sibthorpe +30

We present results from the earliest observations of DEBRIS, a Herschel Key Programme to conduct a volume- and flux-limited survey for debris discs in A-type through M-type stars.…

astro-ph2005★ 51 cited

Multi-Generational Star Formation in L1551

Gerald H. Moriarty-Schieven, Doug Johnstone, John Bally +1

The L1551 molecular cloud contains two small clusters of Class 0 and I protostars, as well as a halo of more evolved Class II and III YSOs, indicating a current and at least one pa…