activity
20022010
most citedFrom Molecular Cores to Planet-forming Disks: A SIRTF Legacy Program

537 citations · 895 across the 8 of their papers we have counts for

collaborators

8 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-ph2006★ 27 cited

The Chemical Evolution of Protoplanetary Disks

E. A. Bergin, Y. Aikawa, G. A. Blake +1

In this review we re-evaluate our observational and theoretical understanding of the chemical evolution of protoplanetary disks. We discuss how improved observational capabilities…

astro-ph2005★ 132 cited

Spitzer Mid-infrared Spectroscopy of Ices Toward Extincted Background Stars

C. Knez, A. C. A. Boogert, K. M. Pontoppidan +6

A powerful way to observe directly the solid state inventory of dense molecular clouds is by infrared spectroscopy of background stars. We present Spitzer/IRS 5-20 micron spectra o…