V* V599 Aur , the SIMBAD biblio

V* V599 Aur , the SIMBAD biblio (23 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST04:31:34

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
2006IBVS.5699....1. 104 0 Observations of variables.
2006IBVS.5700....1M         O           95 1 Reports on new discoveries. MASSIMILIANO M.
2006IBVS.5713....1D 184 20 165. List of timings of minima eclipsing binaries by BBSAG observers. DIETHELM R.
2007IBVS.5781....1D 174 15 166. List of timings of minima eclipsing binaries by BBSAG observers. DIETHELM R.
2009AJ....138..466H viz 15       D               1 4127 116 Automated variable star classification using the Northern Sky Variability Survey. HOFFMAN D.I., HARRISON T.E. and McNAMARA B.J.
2010PASJ...62...81L 1168 T K A D     X C       30 18 1 First R and I lights and their photometric analyses of
GSC 02393-00680. 		LIU L., QIAN S.-B., HE J.-J., et al.
2011IBVS.5969....1K viz 15       D               1 2041 27 The 80th name-list of variable stars. Part I - RA 0h to 6h. KAZAROVETS E.V., SAMUS N.N., DURLEVICH O.V., et al.
2015IBVS.6149....1H 635 57 BAV-Results of observations - Photoelectric Minima of Selected Eclipsing Binaries and Maxima of Pulsating Stars. HUBSCHER J. and LEHMANN P.B.
2016IBVS.6164....1N 85 2 CCD Minima for Selected Eclipsing Binaries in 2015. NELSON R.H.
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.
2019MNRAS.489.2677Z 41           X         1 18 12 V1005 Her: a solar-type shallow-contact binary in a triply fossil system. ZHU L.-Y., WANG Z.H., TIAN X.M., et al.
2020ApJS..249...18C viz 16       D               1 781605 122 The Zwicky Transient Facility catalog of periodic variable stars. CHEN X., WANG S., DENG L., et al.
2020AJ....160...62H viz 3540 T   A D     X C       85 15 9 Long-term photometry and orbital period change of the W UMa-type binary
V0599 Aur: evidence of about 11 yr magnetic-activity cycle. 		HU K., YU Y.-X., ZHANG J.-F., et al.
2020MNRAS.497.2250H viz 16       D               1 620 ~ Very wide companion fraction from Gaia DR2: A weak or no enhancement for hot Jupiter hosts, and a strong enhancement for contact binaries. HWANG H.-C., HAMER J.H., ZAKAMSKA N.L., et al.
2020MNRAS.497.3493Z 16       D               1 360 25 Orbital period cut-off of W UMa-type contact binaries. ZHANG X.-D. and QIAN S.-B.
2021ApJS..254...10L viz 17       D               1 694 37 Statistics of 700 individually studied W UMa stars. LATKOVIC O., CEKI A. and LAZAREVIC S.
2021PASJ...73.1470S 59       D     X         2 59 ~ BM UMa: A middle shallow contact binary at pre-transition stage of evolution from W-type to A-type. SAROTSAKULCHAI T., SOONTHORNTHUM B., POSHYACHINDA S., et al.
2022RAA....22b5011Z 43           X         1 10 1 CSS J075415.6+191052 and NW Leo: Two Contact Binaries at Different Evolutionary Stages. ZHANG X.-D., QIAN S.-B., ZHAO E.-G., 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.
2024AJ....167..192D viz 18       D               1 1374 ~ Detection of Contact Binary Candidates Observed By TESS Using the Autoencoder Neural Network. DING X., SONG Z., WANG C., et al.
2024ApJ...971..113M 45           X         1 5 ~ OO Leo: An Active Contact Binary with Possible Solar-like Differential Rotation. MENG Z.-B., WU P.-R., YU Y.-X., et al.
2026AJ....171...82S 50           X         1 37 ~ A Photometric Study of the Late-type Contact Binary MT Cassiopeiae: A Robust Detection of Three Periodic Eclipse Timing Variations. SONG M.-H., KIM C.-H., LI K., et al.
2026ApJ...997..289W 50           X         1 8 ~ Spectroscopic and Decade-long Photometric Observations of the Contact Binary V2790 Ori: Evidence for a Brown Dwarf Companion and a Solar-like Magnetic Activity Cycle. WANG S.-R., LI K., XIA Q.-Q., et al.

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