HS 0218+3229 , the SIMBAD biblio

HS 0218+3229 , the SIMBAD biblio (24 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.02.21CET06:03:48

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Bibcode/DOI Score in Title|Abstract|
in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
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Title First 3 Authors
2009MNRAS.394L.136M 38           X         1 10 17 Dynamical constraints on the neutron star mass in EXO 0748-676. MUNOZ-DARIAS T., CASARES J., O'BRIEN K., et al.
2009A&A...496..805R 1516 T   A D S O X C       38 15 8 An evolved donor star in the long-period cataclysmic variable
2012Ap.....55..208G 526 T   A S   X         12 4 5 Multicolor photometry of the dwarf nova
HS 0218+3229.
2014ApJ...790...28R 39           X         1 16 7 SDSS J001153.08-064739.2, a cataclysmic variable with an evolved donor in the period gap. REBASSA-MANSERGAS A., PARSONS S.G., COPPERWHEAT C.M., et al.
2015ApJ...808...80C 135       D     X         4 59 53 A FWHM-K2 correlation in black hole transients. CASARES J.
2016MNRAS.460.2526O viz 16       D               1 638 28 Statistical analysis of properties of dwarf novae outbursts. OTULAKOWSKA-HYPKA M., OLECH A. and PATTERSON J.
2017MNRAS.466.2855P 17       D               2 52 64 Effective temperatures of cataclysmic-variable white dwarfs as a probe of their evolution. PALA A.F., GANSICKE B.T., TOWNSLEY D., et al.
2018AJ....156..241H viz 16       D               1 311115 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.
2018PASJ...70...78K 165           X         4 15 3 On the nature of long-period dwarf novae with rare and low-amplitude outbursts. KIMURA M., KATO T., MAEHARA H., et al.
2019MNRAS.489.1023Y 184       D     X C       4 7 ~ A 9-h CV with one outburst in 4 yr of Kepler data. YU Z., THORSTENSEN J.R., RAPPAPORT S., et al.
2020MNRAS.491.5717B viz 43           X         1 202 34 Evidence for reduced magnetic braking in polars from binary population models. BELLONI D., SCHREIBER M.R., PALA A.F., et al.
2020MNRAS.492L..40A viz 17       D               1 1220 31 Disentangling cataclysmic variables in Gaia's HR diagram. ABRIL J., SCHMIDTOBREICK L., EDEROCLITE A., et al.
2020MNRAS.494.1448I viz 17       D               1 291 ~ Inferred time-scales for common envelope ejection using wide astrometric companions. IGOSHEV A.P., PERETS H.B. and MICHAELY E.
2020MNRAS.499..149A 43           X         1 39 14 V1460 Her: a fast spinning white dwarf accreting from an evolved donor star. ASHLEY R.P., MARSH T.R., BREEDT E., et al.
2020PASJ...72...76H 187       D     X C       4 80 11 Spectroscopic properties of the dwarf nova-type cataclysmic variables observed by LAMOST. HAN Z., BOONRUCKSAR S., QIAN S., et al.
2021ApJ...914....5S viz 17       D               1 206 8 Nova-produced common envelope: source of the nonsolar abundances and an additional frictional angular momentum loss in cataclysmic variables. SPARKS W.M. and SION E.M.
2021MNRAS.505.2051E 132           X   F     2 13 18 LAMOST J0140355 + 392651: an evolved cataclysmic variable donor transitioning to become an extremely low-mass white dwarf. EL-BADRY K., QUATAERT E., RIX H.-W., et al.
2021MNRAS.508.4106E 87           X         2 65 22 Birth of the ELMs: a ZTF survey for evolved cataclysmic variables turning into extremely low-mass white dwarfs. EL-BADRY K., RIX H.-W., QUATAERT E., et al.
2021ApJS..257...65S viz 17       D               1 328 5 A catalog of 323 cataclysmic variables from LAMOST DR6. SUN Y., CHENG Z., YE S., et al.
2022MNRAS.516.2455N 18       D               1 287 11 ASAS-SN follow-up of IceCube high-energy neutrino alerts. NECKER J., DE JAEGER T., STEIN R., et al.
2023ApJ...950..139G 1400     A D S   X C       29 34 ~ White Dwarf Photospheric Abundances in Cataclysmic Variables. III. Five Dwarf Novae with an Evolved Secondary Donor Star. GODON P. and SION E.M.
2023MNRAS.523..305T 3919 T K A D S   X C F     81 13 2 The C/N ratio from FUV spectroscopy as a constraint on evolution of the dwarf nova
HS 0218 + 3229.
2023A&A...678A..34B 47           X         1 30 ~ Reversing the verdict: Cataclysmic variables could be the dominant progenitors of AM CVn binaries after all. BELLONI D. and SCHREIBER M.R.
2024ApJ...960...37G 50           X         1 34 ~ White Dwarf Photospheric Abundances in Cataclysmic Variables. IV. Deriving the [N/C] Ratio. GODON P. and SION E.M.

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