Elemental abundances of 4 Lac and nu Cep Virtual Observatory Resource

Authors
  1. Yuce K.
  2. Published by
    CDS
Abstract

Elemental abundance analysis based on high S/N and high resolution Dominion Astrophysical Observatory spectrograms have been performed for two early type supergiants: 4 Lac (B9 Iab) and {nu} Cep (A2 Ia). Lines as weak as of order 5m{AA} are employed in this study. The projected rotational velocities of these stars are 14 and 26km/s, respectively. Both stars show similar radial velocity amplitudes, macroturbulent velocities and the same general elemental abundance trends. Their He, CNO and light element abundances are solar or overabundant while the iron peak and heavy element abundances are solar or underabundant. Detailed LTE model atmosphere abundance analysis shows that 4 Lac has nuclearly processed matter in its photosphere while {nu} Cep does not.

Keywords
  1. supergiant-stars
  2. line-intensities
  3. chemically-peculiar-stars
Bibliographic source Bibcode
2005BaltA..14...51Y
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/BaltA/14/51
IVOA Identifier IVOID
ivo://CDS.VizieR/J/BaltA/14/51

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/BaltA/14/51
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/BaltA/14/51
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/BaltA/14/51
IVOA Table Access TAP
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Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

History

2005-03-12T17:02:26Z
Resource record created
2005-03-12T16:02:35Z
Updated
2005-03-12T17:02:26Z
Created

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