Hot ammonia from NGC 6334I and NGC 6334I(N)

DOI

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.

Identifier
DOI http://doi.org/10.26093/cds/vizier.34660989
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/466/989
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/466/989
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/466/989
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/466/989
Provenance
Creator Beuther H.; Walsh A.J.; Throwirth S.; Zhang Q.; Hunter T.R.; Megeath S.T.,Menten K.M.
Publisher CDS
Publication Year 2008
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Galactic and extragalactic Astronomy; Interstellar medium; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy