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Resource Record Summary

Catalog Service:
C^18^O(1-0) and N_2_H^+^(1-0) in L1495/B213

Short name: J/A+A/554/A55
IVOA Identifier: ivo://CDS.VizieR/J/A+A/554/A55
DOI (Digital Object Identifier): 10.26093/cds/vizier.35540055
Publisher: CDS[+][Pub. ID]
More Info: https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/554/A55
VO Compliance: Level 2: This is a VO-compliant resource.
Status: active
Registered: 2013 Oct 23 09:51:20Z
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Description


Core condensation is a critical step in the star-formation process, but it is still poorly characterized observationally. We have studied the 10pc-long L1495/B213 complex in Taurus to investigate how dense cores have condensed out of the lower density cloud material. We observed L1495/B213 in C^18^O(1-0), N_2_H^+^(1-0), and SO(J_N_=3_2_-2_1_) with the 14m FCRAO telescope, and complemented the data with dust continuum observations using APEX (870um) and IRAM 30m (1200um).

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Developed with the support of the National Science Foundation
under Cooperative Agreement AST0122449 with the Johns Hopkins University
The NAVO project is a member of the International Virtual Observatory Alliance

This NAVO Application is hosted by the Space Telescope Science Institute

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