Hot ammonia from NGC 6334I and NGC 6334I(N) Virtual Observatory Resource

Authors

1. Beuther H.
2. Walsh A.J.
3. Throwirth S.
4. Zhang Q.
5. Hunter T.R.
6. Megeath S.T.,Menten K.M.

Published by

CDS

Abstract

The massive twin cores NGC 6334I and I(N) are in different evolutionary stages and hence ideal targets to study evolutionary variations within the same larger-scale environment. Here, we study the warm, compact gas components. We imaged the two regions with the Australia Telescope Compact Array (ATCA) at high angular resolution in the NH3(3, 3) to (6, 6) inversion lines.

Keywords

1. supernova-remnants
2. early-type-stars
3. astrophysical-masers
4. radio-astronomy
5. interferometry

Bibliographic source Bibcode

2007A&A...466..989B

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/466/989

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/466/989

Document Object Identifer DOI

doi:10.26093/cds/vizier.34660989

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