OGLE BLAP-011 , the SIMBAD biblio

OGLE BLAP-011 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST19:49:59


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Title First 3 Authors
2018MNRAS.477L..30R 98       D       C       2 4 8 On the evolutionary status and pulsations of the recently discovered blue large-amplitude pulsators (BLAPs). ROMERO A.D., CORSICO A.H., ALTHAUS L.G., et al.
2017NatAs...1..166P 16       D               1 16 ~ Blue large-amplitude pulsators as a new class of variable stars. PIETRUKOWICZ P., DZIEMBOWSKI W.A., LATOUR M., et al.
2018MNRAS.478.3871W 297       D     X C       7 14 ~ Which evolutionary status does the Blue Large-Amplitude Pulsators stay at? WU T.
2018A&A...620L...9R 12 ~ Identifying blue large-amplitude pulsators in the Galactic plane using Gaia DR2: a case study. RAMSAY G.
2019ApJS..243...10P 221           X C       2 8 795 Modules for Experiments in Stellar Astrophysics (MESA): pulsating variable stars, rotation, convective boundaries, and energy conservation. PAXTON B., SMOLEC R., SCHWAB J., et al.
2020MNRAS.492..232B 16       D               1 9 ~ Pulsation in faint blue stars. BYRNE C.M. and JEFFERY C.S.
2020MNRAS.496.1105M 41           X         1 9 ~ Confirmation of monoperiodicity above 20 s for two blue large-amplitude pulsators. McWHIRTER P.R., LAM M.C. and STEELE I.A.
2020ApJ...903..100M 83           X         2 9 10 Blue large-amplitude pulsators: the possible surviving companions of Type Ia supernovae. MENG X.-C., HAN Z.-W., PODSIADLOWSKI P., et al.
2022A&A...668A.112X 60       D     X         2 20 2 Shell helium-burning hot subdwarf B stars as candidates for blue large-amplitude pulsators. XIONG H., CASAGRANDE L., CHEN X., et al.
2023ApJ...959...24Z 17       D               1 24 ~ The Formation of Blue Large-amplitude Pulsators from White-dwarf Main-sequence Star Mergers. ZHANG X., JEFFERY C.S., SU J., et al.
2025ApJS..279...21P 19       D               1 45 ~ Observational Parameters of Blue Large-amplitude Pulsators. PIETRUKOWICZ P., LATOUR M., SOSZYNSKI I., et al.
2026ApJ...998..112D 50           X         1 7 ~ New Theoretical Instability Regions, Period-Luminosity Relations, and Masses for Blue Large-amplitude Pulsators. DAS S., JADLOVSKY D. and MOLNAR L.

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