Extremely high-velocity jets in Serpens Virtual Observatory Resource

Authors
  1. Tychoniec L.
  2. Hull C.L.H.
  3. Kristensen L.E.
  4. Tobin J.J.
  5. Le Gouellec V.J.M.,van Dishoeck E.F.
  6. Published by
    CDS
Abstract

ALMA observations of four molecular transitions, CO 2-1, SiO 5-4, H_2_CO 3_03_-2_02_ in Band 6 (ALMA project 2013.1.00726.S; PI: C. Hull) and HCN 1-0 observed in Band 3 (ALMA project 2016.1.00710.S; PI: C. Hull) are presented. The synthesized beam of the observations is between 0.3 and 0.6 arcsec, corresponding to 130-260au at the distance to Serpens Main. The largest recoverable scale in the data is 5 arcsec and 12 arcsec (2150 and 4960au) for Band 3 and Band 6, respectively. The spectral resolution of the observations differs between the spectral windows, ranging from 0.04 to 0.3km/s. For both bands, only 12-m array data were used. The Band 6 data were obtained in two configurations (C43-1 and C43-4 with resolutions of 1.1 and 0.3 arcsec, respectively, and the final images are produced from the combined datasets.

Keywords
  1. young-stellar-objects
  2. protostars
  3. co-line-emission
  4. interstellar-medium
Bibliographic source Bibcode
2019A&A...632A.101T
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/632/A101
IVOA Identifier IVOID
ivo://CDS.VizieR/J/A+A/632/A101
Document Object Identifer DOI
doi:10.26093/cds/vizier.36320101

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History

2019-12-10T09:45:56Z
Resource record created
2019-12-10T08:47:15Z
Updated
2019-12-10T09:45:56Z
Created

Contact

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CDS support team
Postal Address
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
E-Mail
cds-question@unistra.fr