The H2D+ line profile in L 1544.

Details The H2D+ line profile in L 1544. The H2D+ line profile in L 1544.

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005esasp.577..429v&link_type=abstract

In: Proceedings of the dusty and molecular universe: a prelude to Herschel and ALMA, 27-29 October 2004, Paris, France. Ed. by A

Physics

1

Radiative Transfer, Methods: Numerical, Ism: Molecules

Scientific paper

We present radiative transfer models of the H2D+ emission towards the pre-stellar core L 1544. Models with a centrally peaked density distribution come closer to the observed double-peaked lines profile than models with a constant density at the center. However, an additional ingredient such as rotation on <2000 AU scales appears necessary. The effect of (2D) flattening is shown to be minor.

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