Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aas...205.9806d&link_type=abstract
American Astronomical Society Meeting 205, #98.06; Bulletin of the American Astronomical Society, Vol. 36, p.1505
Astronomy and Astrophysics
Astronomy
Scientific paper
We consider the chemical evolution of the envelope surrounding the massive star-forming region AFGL2591. In particular, we extend the previous gas-phase model of Doty et al. (2002) to include grain adsorption/desorption in a more realistic manner, and include evolution of the temperature and luminosity of the central source. While our previous results are generally verified, we find that including these effects brings the space- and time-dependent abundance profiles into even better agreement with observations.
Doty Steven D.
Tan Jian
van Dishoeck Ewine F.
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