Spectroscopy of ups Sgr Virtual Observatory Resource

Authors
  1. Kipper T.
  2. Klochkova V.G.
  3. Published by
    CDS
Abstract

The high resolution spectra of hydrogen-deficient binary {upsilon} Sgr are analyzed. The atmospheric parameters are T_eff_= 12300+/-200K, logg=2.5+/-0.5 and {xi}_t_=5-15km/s depending on the element.

Keywords
  1. be-stars
  2. stellar-atmospheres
  3. chemical-abundances
Bibliographic source Bibcode
2012BaltA..21..219
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/BaltA/21/219
IVOA Identifier IVOID
ivo://CDS.VizieR/J/BaltA/21/219
Document Object Identifer DOI
doi:10.26093/cds/vizier/bm-n-6v

Access

Web browser access HTML
https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/BaltA/21/219
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/BaltA/21/219
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/BaltA/21/219
IVOA Table Access TAP
https://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

History

2013-01-25T14:15:59Z
Resource record created
2013-01-25T14:15:59Z
Created
2026-03-17T20:06:55Z
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