275 citations · 3.6k across the 46 of their papers we have counts for
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Modeling water emission from low-mass protostellar envelopes
T. A. van Kempen, S. D. Doty, E. F. van Dishoeck +2
Within low-mass star formation, water vapor plays a key role in the chemistry and energy balance of the circumstellar material. The Herschel Space Observatory will open up the poss…
A Parameter Study of the Dust and Gas Temperature in a Field of Young Stars
Andrea Urban, Neal J. Evans, Steven D. Doty
We model the thermal effect of young stars on their surrounding environment in order to understand clustered star formation. We take radiative heating of dust, dust-gas collisional…
Infrared Molecular Starburst Fingerprints in Deeply Obscured (U)LIRG Nuclei
F. Lahuis, H. W. W. Spoon, A. G. G. M. Tielens +6
High resolution spectra of the Spitzer Space Telescope show vibration-rotation absorption bands of gaseous C2H2, HCN, and CO2 molecules toward a sample of deeply obscured (U)LIRG n…
Tracing high energy radiation with molecular lines near deeply embedded protostars
P. Stauber, A. O. Benz, J. K. Jorgensen +3
Submillimeter lines of CN, NO, CO+ and SO+, and upper limits on SH+ and N2O are observed with the James Clerk Maxwell Telescope in two high-mass and up to nine low-mass young stell…
Astrochemical confirmation of the rapid evolution of massive YSOs and explanation for the inferred ages of hot cores
S. D. Doty, E. F. van Dishoeck, J. C. Tan
Aims. To understand the roles of infall and protostellar evolution on the envelopes of massive young stellar objects (YSOs). Methods. The chemical evolution of gas and dust is trac…
Water destruction by X-rays in young stellar objects
P. Stauber, J. K. Jorgensen, E. F. van Dishoeck +2
We study the H2O chemistry in star-forming environments under the influence of a central X-ray source and a central far ultraviolet (FUV) radiation field. The gas-phase water chemi…