N131 bubble CO integrated intensity maps

DOI

OB-type stars have strong ionizing radiation and drive energetic winds. The ultraviolet radiation from ionizing stars may heat dust and ionize gas to sweep up an expanding bubble shell. This shell may be the result of feedback leading to a new generation of stars. N131 is an infrared dust bubble residing in a molecular filament. We study the formation and fragmentation of this bubble with multiwavelength dust and gas observations. Towards the bubble N131, we analysed archival multiwavelength observations including 3.6, 4.5, 5.8, 8.0, 24, 70, 160, 250, 350, 500um, 1.1mm, and 21cm. In addition, we performed new observations of CO (2-1), CO (1-0), and ^13^CO (1-0) with the IRAM 30m telescope.

Cone search capability for table J/A+A/585/A117/list (List fo fits images)

Identifier
DOI http://doi.org/10.26093/cds/vizier.35850117
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/585/A117
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/585/A117
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/585/A117
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/585/A117
Provenance
Creator Zhang C.-P.; Li G.-X.; Wyrowski F.; Wang J.-J.; Yuan J.-H.; Xu J.-L.,Gong Y.; Yeh C.C.; Menten K.M.
Publisher CDS
Publication Year 2016
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; Interstellar medium; Natural Sciences; Physics