Asteroseismology of the double-radial mode Scuti star BP Pegasi
arXiv:2203.02722 · doi:10.1093/mnras/stac646
Abstract
Using the ASAS data, we determine the pulsational frequencies of the high-amplitude Sct star BP Pegasi. The analysis revealed only the two known, independent frequencies. On the basis of multicolour Strömgren photometry, we independently find that both frequencies can only be associated with radial modes which, according to the frequency ratio, are fundamental and first overtone modes. The models fitting the two frequencies depend strongly on the opacity data. For low values of the mixing length parameter , only the OPAL seismic models in the post-main sequence phase of evolution are caught within the observed error box. Seismic OP and OPLIB models can only reach the error box if we increase to at least 2.0. Then, including the non-adiabatic parameter into our seismic modelling, we constrain various parameters, employing Monte Carlo-based Bayesian analysis.
16 pages, 15 figures, 6 tables, accepted for publication in MNRAS
References in corpus (7)
- Gaia Early Data Release 3: Parallax bias versus magnitude, colour, and position
- Basic physical parameters of a selected sample of evolved stars
- ADIPLS -- the Aarhus adiabatic oscillation package
- Determining stellar parameters of asteroseismic targets: going beyond the use of scaling relations
- A comprehensive asteroseismic modelling of the high-amplitude delta Scuti star RV Arietis
- Seismic analysis of the double-mode radial pulsator SX Phoenicis
- Mode identification and seismic study of Scuti, the prototype of a class of pulsating stars
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- TESS Observations of Seven Newly Identified High-amplitude Scuti Stars
- Asteroseismology of double-mode radial Scuti stars: AE Ursae Majoris and RV Arietis
- Discovery of resonating integration modes in triple-mode high-amplitude Scuti stars: A new evolutionary phase indicator
- Exploring the unexpected: Disharmonized harmonic pulsation modes in high-amplitude Scuti stars
- Period Variation Rates of Four Radial Single-Mode High-Amplitude Delta Scuti Stars
- Discovery and Characterization of Three New High-amplitude delta Scuti Stars from TESS Observations