activity
20092026
most citedWater in star-forming regions with Herschel (WISH): II. Evolution of 557 GHz 110-101 emission in low-mass protostars

273 citations · 2.3k across the 62 of their papers we have counts for

collaborators
Showing 2013Show all

5 papers · 1 filter

astro-ph.SR2013★ 30 cited

Warm gas towards young stellar objects in Corona Australis - Herschel/PACS observations from the DIGIT key programme

Johan E. Lindberg, Jes K. Jørgensen, Joel D. Green +5

The effects of external irradiation on the chemistry and physics in the protostellar envelope around low-mass young stellar objects are poorly understood. The Corona Australis star…

astro-ph.SR2013★ 56 cited

Far-infrared molecular lines from Low- to High-Mass Star Forming Regions observed with Herschel

A. Karska, F. Herpin, S. Bruderer +13

(Abridged) We study the response of the gas to energetic processes associated with high-mass star formation and compare it with studies on low- and intermediate-mass young stellar…

astro-ph.SR2013★ 88 cited

High-J CO survey of low-mass protostars observed with Herschel-HIFI

Umut A. Yıldız, Lars E. Kristensen, Ewine F. van Dishoeck +8

The evolution of deeply embedded young stellar objects (YSOs) has traditionally been traced through dust continuum spectral energy distributions (SEDs), but the use of CO excitatio…

astro-ph.GA2013★ 126 cited

Embedded Protostars in the Dust, Ice, and Gas In Time (DIGIT) Key Program: Continuum SEDs, and an Inventory of Characteristic Far-Infrared Lines from PACS Spectroscopy

Joel D. Green, Neal J. Evans, Jes K. Jørgensen +17

We present 50-210 um spectral scans of 30 Class 0/I protostellar sources, obtained with Herschel-PACS, and 0.5-1000 um SEDs, as part of the Dust, Ice, and Gas in Time (DIGIT) Key P…

astro-ph.SR2013★ 62 cited

Water in star forming regions with Herschel (WISH) III. Far-infrared cooling lines in low-mass young stellar objects

A. Karska, G. J. Herczeg, E. F. van Dishoeck +22

(Abridged) Far-infrared Herschel-PACS spectra of 18 low-mass protostars of various luminosities and evolutionary stages are studied. We quantify their far-infrared line emission an…