Spectral line identification in 3 Pup Virtual Observatory Resource

Authors
  1. Chentsov E.L.
  2. Klochkova V.G.
  3. Miroshnichenko A.S.
  4. Published by
    CDS
Abstract

Optical spectra taken in 1997-2008 are used to analyze the spectral peculiarities and velocity field in the atmosphere of the peculiar supergiant 3 Pup.

Keywords
  1. Supergiant stars
  2. Spectroscopy
  3. Radial velocity
Bibliographic source Bibcode
2010AstBu...65.150C
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/other/AstBu/65.150
IVOA Identifier IVOID
ivo://CDS.VizieR/J/other/AstBu/65.150

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/other/AstBu/65.150
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/other/AstBu/65.150
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/other/AstBu/65.150
IVOA Table Access TAP
http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

History

2010-06-21T09:53:17Z
Resource record created
2010-06-21T09:53:17Z
Created
2010-08-07T14:03:25Z
Updated

Contact

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