1SWASP J162842.31+101416.7 , the SIMBAD biblio

1SWASP J162842.31+101416.7 , the SIMBAD biblio (23 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST05:01:48


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Title First 3 Authors
2014MNRAS.437.1681M 365       D     X         10 30 85 EL CVn-type binaries - discovery of 17 helium white dwarf precursors in bright eclipsing binary star systems. MAXTED P.F.L., BLOEMEN S., HEBER U., et al.
2014MNRAS.444..208M 6193 T K A D     X C       159 5 31 WASP 1628+10 - an EL CVn-type binary with a very low mass stripped red giant star and multiperiodic pulsations. MAXTED P.F.L., SERENELLI A.M., MARSH T.R., et al.
2016A&A...587L...5C 316           X         8 4 11 Two new pulsating low-mass pre-white dwarfs or SX Phoenicis stars? CORTI M.A., KANAAN A., CORSICO A.H., et al.
2016ApJ...821L..32Z 81           X         2 4 17 Multi-period g-mode pulsations of a pre-He-WD star in the eclipsing binary KIC 9164561. ZHANG X.B., FU J.N., LI Y., et al.
2016A&A...588A..74C 733     A S   X C       17 9 28 Pulsating low-mass white dwarfs in the frame of new evolutionary sequences. CORSICO A.H., ALTHAUS L.G., SERENELLI A.M., et al.
2016ApJ...822L..27G 102     A     X         3 10 16 Discovery of three pulsating, mixed-atmosphere, extremely low-mass white dwarf precursors. GIANNINAS A., CURD B., FONTAINE G., et al.
2016A&A...595L..12I 79             C       3 7 10 Asteroseismic test of rotational mixing in low-mass white dwarfs. ISTRATE A.G., FONTAINE G., GIANNINAS A., et al.
2017MNRAS.467.1874C 120           X         3 14 42 The formation of EL CVn-type binaries. CHEN X., MAXTED P.F.L., LI J., et al.
2018AJ....155....5L 40           X         1 11 7 Absolute properties of the pulsating post-mass transfer eclipsing binary OO Draconis. LEE J.W., HONG K., KOO J.-R., et al.
2018MNRAS.475.2560V 161           X   F     3 58 11 Discovery of 36 eclipsing EL CVn binaries found by the Palomar Transient Factory. VAN ROESTEL J., KUPFER T., RUIZ-CARMONA R., et al.
2018ApJ...858...14S 43           X         1 10 34 Formation of extremely low-mass white dwarf binaries. SUN M. and ARRAS P.
2018A&A...616A..80S 40           X         1 8 3 Comparing the asteroseismic properties of pulsating pre-extremely low mass white dwarf and δ Scuti stars. SANCHEZ ARIAS J.P., ROMERO A.D., CORSICO A.H., et al.
2018A&A...616A.130L 80           X         2 20 3 KIC 8553788: A pulsating Algol with an extreme mass ratio. LIAKOS A.
2018AJ....156..187W 40           X         1 21 6 V1224 Cas: an EL CVn-type eclipsing binary consisting of a helium white dwarf precursor and a delta Scuti pulsator. WANG K., LUO C., ZHANG X., et al.
2018AJ....156..241H viz 16       D               1 311106 199 A first catalog of variable stars measured by the Asteroid Terrestrial-impact Last Alert System (ATLAS). HEINZE A.N., TONRY J.L., DENNEAU L., et al.
2019ApJ...884..165Z 43           X         1 5 10 Discovery and seismic analysis of an EL CVn-type binary with hybrid δ Sct-γ Dor pulsations. ZHANG X.B., WANG K., CHEN X.H., et al.
2020A&A...642A..91L 16       D               1 61 10 Asteroseismology of two Kepler detached eclipsing binaries. LIAKOS A.
2021AJ....161..137H 84           X         2 10 6 The pre-He white dwarfs in eclipsing binaries. II. WASP 0843-11. HONG K., LEE J.W., KOO J.-R., et al.
2023ApJS..266...14T viz 17       D               1 21501 ~ A New Catalog of Am-type Chemically Peculiar Stars Based on LAMOST. TIAN X.-M., WANG Z.-H., ZHU L.-Y., et al.
2023A&A...674A..16M viz 17       D               1 2184478 19 Gaia Data Release 3 The first Gaia catalogue of eclipsing-binary candidates. MOWLAVI N., HOLL B., LECOEUR-TAIBI I., et al.
2023MNRAS.525.2605G 148       D     X   F     3 73 ~ The white dwarf mass-orbital period relation under wind mass-loss. GAO S.-J. and LI X.-D.
2024MNRAS.533.2058C 90           X         2 14 ~ Empirical instability strip for pre-He WD in EL CVn type binary systems. CAKIRLI O., HOYMAN B. and OZDARCAN O.
2025MNRAS.539..967C 47           X         1 7 ~ Two additional members of a newly identified group of pulsating pre-He white dwarfs. CAKIRLI O. and HOYMAN B.

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