Molecular and atomic gas in the LMC. II.

DOI

We compare the CO (J=1-0) and HI emission in the Large Magellanic Cloud in three dimensions, i.e., including a velocity axis in addition to the two spatial axes, with the aim of elucidating the physical connection between giant molecular clouds (GMCs) and their surrounding HI gas. The CO(J=1-0) data set is from the second NANTEN CO survey (Fukui et al. 2008, Cat. J/ApJS/178/56) and the HI data set is from the merged Australia Telescope Compact Array (ATCA) and Parkes Telescope surveys (Kim et al. 2003ApJS..148..473K).

Cone search capability for table J/ApJ/705/144/table2 (List of selected 123 giant molecular clouds (GMCs))

Identifier
DOI http://doi.org/10.26093/cds/vizier.17050144
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/ApJ/705/144
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/705/144
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/705/144
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/ApJ/705/144
Provenance
Creator Fukui Y.; Kawamura A.; Wong T.; Murai M.; Iritani H.; Mizuno N.; Mizuno Y.,Onishi T.; Hughes A.; Ott J.; Muller E.; Staveley-Smith L.; Kim S.
Publisher CDS
Publication Year 2011
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