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19952004
most citedChemical changes during star formation: high- versus low-mass YSOs

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astro-ph2004

X-ray Chemistry in the Envelopes around Young Stellar Objects

P. Staeuber, A. O. Benz, S. D. Doty +1

We have studied the influence of X-rays from a massive young stellar object (YSO) on the chemistry of its own envelope by extending the models of Doty et al. (2002) and Staeuber et…

astro-ph2004

A submillimeter line survey of low-mass protostars: prelude to ALMA and Herschel

E. F. van Dishoeck, J. K. Joergensen, S. Maret +5

The results from a single-dish molecular line survey of a set of 18 deeply embedded young stellar objects are summarized. More than 40 lines from 16 different species were observed…

astro-ph2003

On the Feasibility of Disk Chemical Modeling

Dmitry Semenov, Yaroslav Pavluchenkov, Thomas Henning +2

In this paper, we compare the results of the modeling of a protoplanetary disk chemical evolution obtained with the UMIST95 and ``New Standard Model'' (NSM) chemical databases. Ass…

astro-ph20031 cited

Chemical changes during star formation: high- versus low-mass YSOs

Ewine F. van Dishoeck

Recent observational studies of high- and low-mass YSOs at (sub)millimeter and infrared wavelengths are reviewed, and chemical diagnostics of the different physical components are…

astro-ph2002

Results from a VLT-ISAAC survey of ices and gas around young stellar objects

K. M. Pontoppidan, H. Fraser, F. L. Schoeier +3

General results from a 3-5 micron spectroscopic survey of nearby low-mass young stellar objects are presented. L and M-band spectra have been obtained of \~50 low mass embedded you…

astro-ph2002

Molecular abundances in low-mass protostellar envelopes

Jes K. Jorgensen, Fredrik L. Schoeier, Ewine F. van Dishoeck

A study of the chemical structure of the envelopes around a sample protostars is introduced. Physical models for the envelopes derived using 1D radiative transfer modeling of their…