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Resource Record Summary

Catalog Service:
Chamaeleon-MMS1 NH_3_ (1,1) and (2,2) maps

Short name: J/A+A/564/A99
IVOA Identifier: ivo://CDS.VizieR/J/A+A/564/A99
DOI (Digital Object Identifier): 10.26093/cds/vizier.35640099
Publisher: CDS[+][Pub. ID]
More Info: https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/564/A99
VO Compliance: Level 2: This is a VO-compliant resource.
Status: active
Registered: 2014 Apr 11 09:12:12Z
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Description


The aim of this study is to investigate the structure and kinematics of the nearby candidate first hydrostatic core Cha-MMS1. Cha-MMS1 was mapped in the NH_3_(1,1) line and the 1.2cm continuum using the Australia Telescope Compact Array, ATCA. The angular resolution of the ATCA observations is 7" (~1000AU), and the velocity resolution is 50m/s. The core was also mapped with the 64-m Parkes telescope in the NH_3_(1,1) and (2,2) lines. Observations from Herschel Space Observatory and Spitzer Space telescope were used to help interpretation. The ammonia spectra were analysed using Gaussian fits to the hyperfine structure. A two-layer model was applied in the central parts of the core where the ATCA spectra show signs of self-absorption.

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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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