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2000ApJ...536..845M - Astrophys. J., 536, 845-856 (2000/June-3)
A spectral line study of Serpens S68 FIRS1 region.
McMULLIN J.P., MUNDY L.G., BLAKE G.A., WILKING B.A., MANGUM J.G. and LATTER W.B.
Abstract (from CDS):
Overall, the combined properties and measured abundances suggest an intermediate state between the extremes of dark clouds and evolved warm cores like Orion KL. In general, the Serpens NW condensation appears very similar to the IRAS 16293-2422 region, which is itself an example of a cool, low-mass star-forming region with chemical tracers characteristic of hotter, higher mass regions. Our results support the suggestion that the general chemical morphology of a region is determined more by the age of the region than by its mass.
Abstract Copyright: ∼
Journal keyword(s): ISM: Abundances - ISM: individual (S68) - ISM: Molecules - Radio Continuum: ISM - Stars: Formation
Simbad objects: 15
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