Search Results - "Rawlings, J.M.C."

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  1. 1

    Observational Indicators of Formation Excitation of H2 by Tiné, S, Williams, Da, Clary, Dc, Farebrother, Aj, Fisher, Aj, Meijer, Ajhm, Rawlings, Jmc, Davis, Cj

    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…”
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    Journal Article
  2. 2

    Modeling the Physical Structure of the Low-Density Pre-Protostellar Core Lynds 1498 by Shirley, Yancy L, Nordhaus, Miranda K, Grcevich, Jana M, Evans II, Neal J, Rawlings, Jonathan M. C, Tatematsu, Ken’ichi

    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…”
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    Modelling line profiles in infalling cores by Rawlings, J.M.C., Yates, J.A.

    “…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…”
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  5. 5

    Molecular Clouds as Ensembles of Transient Cores by Garrod, R. T, Williams, D. A, Rawlings, J. M. C

    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,…”
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    Chemical effects of H2 formation excitation by Garrod, Rt, Rawlings, Jmc, Williams, Da

    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^…”
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  8. 8

    The chemistry of transient dense cores by Garrod, R. T., Williams, D. A., Hartquist, T. W., Rawlings, J. M. C., Viti, S.

    “…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…”
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