Probing the Initial Conditions of Clustered Star Formation -- Large Scale On-the-Fly Mapping of Orion B at FCRAO

dc.creatorRidge, Naomi A.
dc.creatorBergin, Edwin A.
dc.creatorMegeath, S. T.
dc.date2002-05-24
dc.date.accessioned2026-07-07T02:03:46Z
dc.date.available2026-07-07T02:03:46Z
dc.descriptionIn order to obtain a census of the pre-stellar and star-forming molecular cores, we have begun an unbiased survey in CS and N2H+ of the L1630 and L1641 molecular clouds. The use of these two molecular species enables us to quantify and disentangle the effects of depletion often seen in CS observations of dense cores. The spectral line data will provide essential kinematical information not present in similar studies of the sub-millimeter dust-continuum, enabling us to examine the overall core to core velocity dispersion and study the effects of infall and outflows around known sub-mm and infra-red sources. Here we present our initial observations of part of L1630, taken during the commissioning phase of the FCRAO On-the-Fly Mapping system in January 2002.
dc.description5 pages, 3 figures, to appear in the ASP Conference Proceedings, "Galactic Star Formation Across the Stellar Mass Spectrum"
dc.identifierhttps://arxiv.org/abs/astro-ph/0205432
dc.identifierhttp://arxiv.org/abs/astro-ph/0205432
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4501
dc.subjectAstrophysics
dc.titleProbing the Initial Conditions of Clustered Star Formation -- Large Scale On-the-Fly Mapping of Orion B at FCRAO
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