Search Results - "Rawlings, J.M.C."
-
1
Observational Indicators of Formation Excitation of H2
Published in Astrophysics and space science (2003)“…Theoretical predictions by Farebrother et al. and Meijer et al. of rovibrational excitation probabilities in H^sub 2^ arising from formation by Eley-Rideal…”
Get full text
Journal Article -
2
Modeling the Physical Structure of the Low-Density Pre-Protostellar Core Lynds 1498
Published in The Astrophysical journal (20-10-2005)“…Pre-protostellar cores likely represent the incipient stages of low-mass (-1 M sub( )) star formation. Lynds 1498 is a pre-protostellar core (PPC) and was one…”
Get full text
Journal Article -
3
Modelling line profiles in infalling cores
Published in Monthly notices of the Royal Astronomical Society (01-10-2001)Get full text
Journal Article -
4
Modelling line profiles in infalling cores
Published in Monthly notices of the Royal Astronomical Society (01-10-2001)“…Results are presented from a model of molecular line formation in collapsing star-forming cores. The study includes, for the first time, a self-consistent…”
Get full text
Journal Article -
5
Molecular Clouds as Ensembles of Transient Cores
Published in The Astrophysical journal (20-02-2006)“…We construct models of molecular clouds that are considered ensembles of transient cores. Each core is assumed to develop in the background gas of the cloud,…”
Get full text
Journal Article -
6
Observational Indicators of Formation Excitation of H 2
Published in Astrophysics and space science (2003)Get full text
Journal Article -
7
Chemical effects of H2 formation excitation
Published in Astrophysics and space science (2003)“…The effects of the production on dust grain surfaces of molecular hydrogen in excited states have been investigated. On the assumption that all of the H^sub 2^…”
Get full text
Journal Article -
8
The chemistry of transient dense cores
Published in Monthly notices of the Royal Astronomical Society (11-01-2005)“…We investigate the chemistry of a transient density fluctuation, with properties similar to those of a dense core within a molecular cloud. We run a multipoint…”
Get full text
Journal Article