On the multiperiodicity of the δ Scuti star BDS 1269A (VW Arietis). The fifth campaign of STEPHI network in 1993.

Bibcode
1996A&AS..120..179L
Liu, Y. Y.; Jiang, S. Y.; Michel, E.; Hernandez, M. M.; Chevreton, M.; Auvergne, M.; Mangeney, A.; Belmonte, J. A.; Goupil, M. J.; Baglin, A.; Roca-Cortés, T.; Vidal, I.
Referencia bibliográfica

Astronomy and Astrophysics Supplement, v.120, p.179-186

Fecha de publicación:
11
1996
Número de autores
12
Número de autores del IAC
1
Número de citas
9
Número de citas referidas
5
Descripción
This paper reports on the fifth STEPHI multi-site photometric campaign in 1993 devoted to the δ Scuti star BDS 1269A (VW Ari). The observation yielded a data set of 150.7 hours. Our analysis has resulted in 7 identified frequencies. These frequencies exhibit three couple-frequency character, and also fit the previous investigations quite well. An attempt to identify the pulsation modes is made, but no equidistant evidence can be detected, and a second-order effect for rotational splitting has to be considered to explain the complicated nature of BDS 1269A.
Tipo
Con árbitro

Te puede interesar

  • Con árbitro
    Expanded Sample of Small Magellanic Cloud Ultraviolet Dust Extinction Curves: Correlations between the 2175 Å Bump, q <SUB>PAH</SUB>, Ultraviolet Extinction Shape, and N(H I)/A(V)
    The Small Magellanic Cloud (SMC) shows a large variation in ultraviolet (UV) dust extinction curves, ranging from Milky Way (MW) like to significantly steeper curves with no detectable 2175 Å bump. This result is based on a sample of only nine sight lines. From Hubble Space Telescope Space Telescope Imaging Spectrograph and IUE spectra of OB stars
    Gordon, Karl D. et al.

    Fecha de publicación:

    7
    2024
    Bibcode
    2024ApJ...970...51G
  • Con árbitro
    Age of Massive Galaxies at Redshift 8
    Recent James Webb Space Telescope data analyses have shown that massive red galaxies existed at redshifts z ≳ 6, a discovery that is difficult to understand in the context of standard cosmology (ΛCDM). Here, we analyze these observations more deeply, by fitting a stellar population model to the optical and near-infrared photometric data. These fits
    López-Corredoira, M. et al.

    Fecha de publicación:

    7
    2024
    Bibcode
    2024ApJ...970...63L
  • Con árbitro
    Early Results from the HUMDRUM Survey: A Small, Earth-mass Planet Orbits TOI-1450A
    M-dwarf stars provide us with an ideal opportunity to study nearby small planets. The HUnting for M Dwarf Rocky planets Using MAROON-X (HUMDRUM) survey uses the MAROON-X spectrograph, which is ideally suited to studying these stars, to measure precise masses of a volume-limited (<30 pc) sample of transiting M-dwarf planets. TOI-1450 is a nearby (22
    Brady, Madison et al.

    Fecha de publicación:

    8
    2024
    Bibcode
    2024AJ....168...67B
    Número de citas
    0