Abundant H$\mathsf{_{2}}$D$\mathsf{^{+}}$ in the pre–stellar core L1544
Open Access
- 23 May 2003
- journal article
- Published by EDP Sciences in Astronomy & Astrophysics
- Vol. 403 (3) , L37-L41
- https://doi.org/10.1051/0004-6361:20030526
Abstract
Astronomy & Astrophysics (A&A) is an international journal which publishes papers on all aspects of astronomy and astrophysicsKeywords
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This publication has 34 references indexed in Scilit:
- CO Depletion and Deuterium Fractionation in Prestellar CoresThe Astrophysical Journal, 2003
- Deuterated molecules as a probe of ionization fraction in dense interstellar cloudsPlanetary and Space Science, 2002
- Deuterium fractionation on interstellar grains studied with modified rate equations and a Monte Carlo approachPlanetary and Space Science, 2002
- The degree of CO depletion in pre-stellar coresAstronomy & Astrophysics, 2002
- N[TINF]2[/TINF]H[TSUP]+[/TSUP] and C[TSUP]18[/TSUP]O Depletion in a Cold Dark CloudThe Astrophysical Journal, 2002
- Molecular Evolution in Collapsing Prestellar CoresThe Astrophysical Journal, 2001
- Protostars and Planets IVIcarus, 2000
- Chemical Evolution in Preprotostellar and Protostellar CoresThe Astrophysical Journal, 1997
- A search for the rotational transitions of H2D+ at 1370 GHz and H3O+ at 985 GHzThe Astrophysical Journal, 1993
- Interstellar absorption lines toward NGC 2264 and AFGL 2591 - Abundances of H2, H3(+), and COThe Astrophysical Journal, 1990