Molecular clouds and star formation

DOI

As a part of the Milky Way Imaging Scroll Painting (MWISP) survey, the aim is to study the physical properties of molecular clouds and their associated star formation toward the Galactic plane within 216.25{deg}<=l<=218.75{deg} and -0.75{deg}<=b<=1.25{deg}, which covers the molecular cloud complex S287. Using the 3x3 Superconducting Spectroscopic Array Receiver (SSAR) at the PMO-13.7m telescope, we performed a simultaneous ^12^CO (1-0), ^13^CO (1-0), C^18^O (1-0) mapping toward molecular clouds in a region encompassing 3.75 square degrees. The beam size is 52" for ^12^CO (1-0) and 55" for ^13^CO (1-0) and C^18^O (1-0).

Cone search capability for table J/A+A/588/A104/list (List of fits datacubes)

Cone search capability for table J/A+A/588/A104/tabled1 (The infrared photometric magnitudes of identified YSO candidates in the surveyed region)

Identifier
DOI http://doi.org/10.26093/cds/vizier.35880104
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/588/A104
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/588/A104
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/588/A104
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/588/A104
Provenance
Creator Gong Y.; Mao R.Q.; Fang M.; Zhang S.B.; Su Y.; Yang J.; Jiang Z.B.; Xu Y.,Wang M.; Wang Y.; Lu D.R.; Sun J.X.
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; Galactic and extragalactic Astronomy; Interstellar medium; Natural Sciences; Physics; Stellar Astronomy