SX Phe Virtual Observatory Resource

Authors
  1. KIM C.
  2. MCNAMARA D.H.
  3. CHRISTENSEN C.G.
  4. Published by
    CDS
Abstract

Simultaneous photometric (uvbyBeta) and spectrographic observations of SX Phe are described. Analysis of the light and velocity frequency spectra are performed. It is shown that all frequencies detected are harmonics or combinations of the fundamental and first harmonic frequencies. Intrinsic (b-y) and c1 values used in conjunction with a model-atmosphere grid appropriate for a star with [M/H]=-1.0 yields <Teff>=7360K and <logg>=3.90. Standard evolutionary models indicate the mass is 1.13 M_{sun}_ and <Mv> value is +2.9. The radial-velocity data indicate a mean radial velocity of -37km/s and a total range of 38km/s. Addresses: Kim C. kimastro@garam.kreonet.re.kr Department of Earth Science Education, Chonbuk National University, Korea McNarama D.H. and Christiensen C.G. pasp@astro.byu.edu Department of Physics and Astronomy, Brigham Young University, Provo, Utah 84602

Keywords
  1. variable-stars
  2. visible-astronomy
  3. medium-band-photometry
  4. radial-velocity
Bibliographic source Bibcode
1993AJ....106.2493K
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/106/2493
IVOA Identifier IVOID
ivo://CDS.VizieR/J/AJ/106/2493
Document Object Identifer DOI
doi:10.26093/cds/vizier.51062493

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/106/2493
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/106/2493
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/106/2493
IVOA Table Access TAP
http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

History

1997-12-09T20:13:21Z
Resource record created
1997-12-09T20:13:21Z
Created
2023-04-06T16:50:04Z
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