SDSS J105754.25+275947.5 , the SIMBAD biblio

SDSS J105754.25+275947.5 , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST01:07:23


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Title First 3 Authors
2009AJ....137.4011S 15       D               2 44 69 Cataclysmic variables from SDSS. VII. The seventh year. SZKODY P., ANDERSON S.F., HAYDEN M., et al.
2012AJ....144...81T viz 15       D               1 337 25 Spectroscopy and photometry of cataclysmic variable candidates from the Catalina Real Time Survey. THORSTENSEN J.R. and SKINNER J.N.
2013MNRAS.431.1800W 16       D               1 35 10 Mining unusual and rare stellar spectra from large spectroscopic survey data sets using the outlier-detection method. WEI P., LUO A., LI Y., et al.
2015A&A...573A..61S viz 953     A D S O X C       23 18 5 Orbital periods of cataclysmic variables identified by the SDSS. IX. NTT photometry of eight eclipsing and three magnetic systems. SOUTHWORTH J., TAPPERT C., GAENSICKE B.T., et al.
2017MNRAS.467.1024M 1746 T K A D S   X C F     40 14 3
SDSS J105754.25+275947.5: a period-bounce eclipsing cataclysmic variable with the lowest-mass donor yet measured.
McALLISTER M.J., LITTLEFAIR S.P., DHILLON V.S., et al.
2017PASJ...69...75K viz 41           X         1 98 34 Survey of period variations of superhumps in SU UMa-type dwarf novae. IX. The ninth year (2016-2017). KATO T., ISOGAI K., HAMBSCH F.-J., et al.
2019MNRAS.482.4570G viz 17       D               1 486647 296 A Gaia Data Release 2 catalogue of white dwarfs and a comparison with SDSS. GENTILE FUSILLO N.P., TREMBLAY P.-E., GANSICKE B.T., et al.
2018PASJ...70...47K 99       D       C       3 27 3 ASASSN-16dt and ASASSN-16hg: Promising candidate period bouncers. KIMURA M., ISOGAI K., KATO T., et al.
2019MNRAS.484.2566L 17       D               1 27 4 Signs of accretion in the white dwarf + brown dwarf binary NLTT5306. LONGSTAFF E.S., CASEWELL S.L., WYNN G.A., et al.
2019MNRAS.486.2169K viz 17       D               2 25030 80 White dwarf and subdwarf stars in the Sloan Digital Sky Survey Data Release 14. KEPLER S.O., PELISOLI I., KOESTER D., et al.
2019MNRAS.486.5535M viz 17       D               2 54 41 The evolutionary status of Cataclysmic Variables: eclipse modelling of 15 systems. McALLISTER M., LITTLEFAIR S.P., PARSONS S.G., et al.
2020AJ....159...35W 43           X         1 6 ~ Photometric and spectroscopic studies of superoutbursts of three dwarf novae independently identified by the SVOM/GWAC system in 2018. WANG J., LI H.L., XIN L.P., et al.
2020AJ....159...43H viz 17       D               1 182 17 Spectroscopically identified cataclysmic variables from the LAMOST survey. I. The sample. HOU W., LUO A.-L., LI Y.-B., et al.
2020MNRAS.491.5717B viz 17       D               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.
2021ApJ...914....5S viz 104       D       C       2 206 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.
2021ApJ...918...58A 104       D       C       2 22 5 Period bouncer cataclysmic variable EZ Lyn in quiescence. AMANTAYEVA A., ZHARIKOV S., PAGE K.L., et al.
2021MNRAS.508.3877G viz 17       D               3 451937 102 A catalogue of white dwarfs in Gaia EDR3. GENTILE FUSILLO N.P., TREMBLAY P.-E., CUKANOVAITE 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.
2023MNRAS.524.4867I viz 19       D               1 99 ~ A catalogue of cataclysmic variables from 20 yr of the Sloan Digital Sky Survey with new classifications, periods, trends, and oddities. INIGHT K., GANSICKE B.T., BREEDT E., et al.
2023A&A...679L...8S 19       D               1 23 ~ Period bouncers as detached magnetic cataclysmic variables. SCHREIBER M.R., BELLONI D. and VAN ROESTEL J.

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