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| Query : 2013MNRAS.428.3034S |
2013MNRAS.428.3034S - Mon. Not. R. Astron. Soc., 428, 3034-3047 (2013/February-1)
Pulsation models for the 0.26 M☉ star mimicking RR Lyrae pulsator. Model survey for the new class of variable stars.
SMOLEC R., PIETRZYNSKI G., GRACZYK D., PILECKI B., GIEREN W., THOMPSON I., STEPIEN K., KARCZMAREK P., KONORSKI P., GORSKI M., SUCHOMSKA K., BONO G., PRADA MORONI P.G. and NARDETTO N.
Abstract (from CDS):
We conduct a model survey for the new class of low-mass pulsators similar to OGLE-BLG-RRLYR-02792 - products of evolution in the binary systems. We compute a grid of models with masses corresponding to half (or less) of the typical mass of RR Lyrae variable, 0.20 ≤ M ≤ 0.30M☉, and discuss the properties of the resulting light and radial velocity curves. Resonant bump progression is clear and may be used to distinguish such stars from classical RR Lyrae stars. We present the Fourier decomposition parameters for the modelled light and radial velocity curves. The expected values of the φ31 Fourier phase for the light curves differ significantly from that observed in RR Lyrae stars, which is another discriminant of the new class.
Abstract Copyright: © 2012 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2012)
Journal keyword(s): hydrodynamics - methods: numerical - binaries: eclipsing - stars: oscillations - stars: variables: RR Lyrae
Simbad objects: 2
| Number of rows : 2 |
| N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2026 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | OGLE BLG-RRLYR-2792 | RR* | 17 47 38.2072195464 | -35 31 07.163702436 | 17.079 | 15.734 | ~ | 46 | 0 | |||
| 2 | NAME Galactic Bulge | reg | ~ | ~ | ~ | 4794 | 0 |
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