Gas-grain chemical models of star-forming molecular clouds as constrained by ISO and SWAS observations
Open Access
- 15 November 2001
- journal article
- Published by EDP Sciences in Astronomy & Astrophysics
- Vol. 378 (3), 1024-1036
- https://doi.org/10.1051/0004-6361:20011193
Abstract
Astronomy & Astrophysics (A&A) is an international journal which publishes papers on all aspects of astronomy and astrophysicsKeywords
This publication has 60 references indexed in Scilit:
- Implications of [ITAL]Submillimeter Wave Astronomy Satellite[/ITAL] Observations for Interstellar Chemistry and Star FormationThe Astrophysical Journal, 2000
- The Composition and Distribution of Dust along the Line of Sight toward the Galactic CenterThe Astrophysical Journal, 2000
- Formation of Interstellar Ices behind Shock WavesThe Astrophysical Journal, 1999
- The Postshock Chemical Lifetimes of Outflow Tracers and a Possible New Mechanism to Produce Water Ice MantlesThe Astrophysical Journal, 1998
- Chemical models of interstellar gas-grain processes -- III. Molecular depletion in NGC 2024Monthly Notices of the Royal Astronomical Society, 1997
- Chemical Evolution in Preprotostellar and Protostellar CoresThe Astrophysical Journal, 1997
- Density Structure in Giant Molecular Cloud CoresThe Astrophysical Journal, 1996
- Chemical limit cycles for models of a region of low-mass star formationMonthly Notices of the Royal Astronomical Society, 1988
- Mass loaded astronomical flows – II. The chemistry in T-Tauri wind-blown bubbles in dense molecular cloudsMonthly Notices of the Royal Astronomical Society, 1988
- Molecular abundances in OMC-1 - The chemical composition of interstellar molecular clouds and the influence of massive star formationThe Astrophysical Journal, 1987