most citedHerschel-HIFI observations of high-J CO lines in the NGC 1333 low-mass star-forming region

53 citations · 107 across the 3 of their papers we have counts for

collaborators

21 papers

astro-ph.EP2013

The D/H ratio in the atmospheres of Uranus and Neptune from Herschel PACS observations

H. Feuchtgruber, E. Lellouch, G. Orton +9

Herschel-PACS measurements of the rotational R(0) and R(1) HD lines in the atmospheres of Uranus and Neptune are analyzed in order to derive a D/H ratio with improved precision for…

astro-ph.GA2010

Water in Star-Forming Regions with the Herschel Space Observatory (WISH): Overview of key program and first results

E. F. van Dishoeck, L. E. Kristensen, A. O. Benz +12

`Water In Star-forming regions with Herschel' (WISH) is a key program on the Herschel Space Observatory designed to probe the physical and chemical structure of young stellar objec…

astro-ph.SR2010★ 53 cited

Herschel-HIFI observations of high-J CO lines in the NGC 1333 low-mass star-forming region

U. A. Yıldız, E. F. van Dishoeck, L. E. Kristensen +60

Herschel-HIFI observations of high-J lines (up to J_u=10) of 12CO, 13CO and C18O are presented toward three deeply embedded low-mass protostars, NGC 1333 IRAS 2A, IRAS 4A, and IRAS…

astro-ph.EP2010★ 24 cited

First results on Martian carbon monoxide from Herschel/HIFI observations

P. Hartogh, M. I. Błęcka, C. Jarchow +48

We report on the initial analysis of Herschel/HIFI carbon monoxide (CO) observations of the Martian atmosphere performed between 11 and 16 April 2010. We selected the (7-6) rotatio…

astro-ph.GA2010

Variations in H2O+/H2O ratios toward massive star-forming regions

F. Wyrowski, F. van der Tak, F. Herpin +63

Early results from the Herschel Space Observatory revealed the water cation H2O+ to be an abundant ingredient of the interstellar medium. Here we present new observations of the H2…

astro-ph.GA2010

Water abundances in high-mass protostellar envelopes: Herschel observations with HIFI

M. Marseille, F. F. S. van der Tak, F. Herpin +4

We derive the dense core structure and the water abundance in four massive star-forming regions which may help understand the earliest stages of massive star formation. We present…