273 citations · 2k across the 34 of their papers we have counts for
34 papers
WISH VI. Constraints on UV and X-ray irradiation from a survey of hydrides in low- to high-mass YSOs
A. O. Benz, S. Bruderer, E. F. van Dishoeck +18
Hydrides are simple compounds containing one or a few hydrogen atoms bonded to a heavier atom. They are fundamental precursor molecules in cosmic chemistry and many hydride ions ha…
Water in star-forming regions with Herschel (WISH) V. The physical conditions in low-mass protostellar outflows revealed by multi-transition water observations
J. C. Mottram, L. E. Kristensen, E. F. van Dishoeck +17
Context: Outflows are an important part of the star formation process as both the result of ongoing active accretion and one of the main sources of mechanical feedback on small sca…
Dense molecular cocoons in the massive protocluster W3 IRS5: a test case for models of massive star formation
K. -S. Wang, T. L. Bourke, M. R. Hogerheijde +4
[Context] Two competing models describe the formation of massive stars in objects like the Orion Trapezium. In the turbulent core accretion model, the resulting stellar masses are…
Observational evidence for dissociative shocks in the inner 100 AU of low-mass protostars using Herschel-HIFI
L. E. Kristensen, E. F. van Dishoeck, A. O. Benz +3
Herschel-HIFI spectra of H2O towards low-mass protostars show a distinct velocity component not seen in observations from the ground of CO or other species. The aim is to character…
Water in star-forming regions with Herschel (WISH). IV. A survey of low-J H2O line profiles toward high-mass protostars
Floris van der Tak, Luis Chavarria, Fabrice Herpin +4
To understand the origin of water line emission and absorption during high-mass star formation, we decompose high-resolution Herschel-HIFI line spectra toward 19 high-mass star-for…
OH far-infrared emission from low- and intermediate-mass protostars surveyed with Herschel-PACS
S. F. Wampfler, S. Bruderer, A. Karska +10
OH is a key species in the water chemistry of star-forming regions, because its presence is tightly related to the formation and destruction of water. This paper presents OH observ…