IRAS 16293-2422 ALMA maps

DOI

We focus on the kinematical properties of a proto-binary to study the infall and rotation of gas toward its two protostellar components. We present ALMA Science Verification observations with high-spectral resolution of IRAS 16293-2422 at 220.2GHz. The wealth of molecular lines in this source and the very high spectral resolution offered by ALMA allow us to study the gas kinematics with unprecedented detail.

Cone search capability for table J/A+A/544/L7/list (List of FITS files)

Identifier
DOI http://doi.org/10.26093/cds/vizier.35449007
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/544/L7
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/544/L7
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/544/L7
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/544/L7
Provenance
Creator Pineda J.E.; Maury A.J.; Fuller G.A.; Testi L.; Garcia-Appadoo D.,Peck A.B.; Villard E.; Corder S.A.; van Kempen T.A.; Turner J.L.,Tachihara K.; Dent W.
Publisher CDS
Publication Year 2012
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; Cosmology; Interstellar medium; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy