HS 0229+8016 , the SIMBAD biblio

HS 0229+8016 , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST01:10:10

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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
2001PASP..113..764D viz 1714 277 A catalog and atlas of cataclysmic variables: the living edition. DOWNES R.A., WEBBINK R.F., SHARA M.M., et al.
2005A&A...443..995A 110 T K                 21 24 HS 0139+0559,
HS 0229+8016, HS 0506+7725, and HS 0642+5049: four new long-period cataclysmic variables. 		AUNGWEROJWIT A., GAENSICKE B.T., RODRIGUEZ-GIL P., et al.
2005ASPC..330..469A 3 0 Three new long-period CVs from the Hamburg Quasar Survey. AUNGWEROJWIT A., GAENSICKE B.T., RODRIGUEZ-GIL P., et al.
2006A&A...455..659A 65 26 Dwarf novae in the Hamburg quasar survey: rarer than expected. AUNGWEROJWIT A., GAENSICKE B.T., RODRIGUEZ-GIL P., et al.
2007MNRAS.374.1359R 26 35 Spectroscopic search for new SW Sextantis stars in the 3-4 h orbital period range - I. RODRIGUEZ-GIL P., SCHMIDTOBREICK L. and GANSICKE B.T.
2008NewA...13..133A viz 15       D               459 29 Spatial distribution and galactic model parameters of cataclysmic variables. AK T., BILIR S., AK S., et al.
2010NewA...15..491A 15       D               2 196 9 The age of cataclysmic variables: A kinematical study. AK T., BILIR S., AK S., et al.
2012NewA...17..570R 38           X         1 7 2 The photometric period and variability of the cataclysmic variable V849 Herculis (PG 1633+115). RINGWALD F.A., RUDE II G.D., ROVETO J.J., et al.
2013NewA...22....7A 15       D               1 160 5 Population types of cataclysmic variables in the solar neighbourhood. AK T., BILIR S., GUVER T., et al.
2019A&A...621A..38G viz 16       D               1 39805 85 The population of hot subdwarf stars studied with Gaia. II. The Gaia DR2 catalogue of hot subluminous stars. GEIER S., RADDI R., GENTILE FUSILLO N.P., et al.
2020MNRAS.492L..40A viz 16       D               1 1220 31 Disentangling cataclysmic variables in Gaia's HR diagram. ABRIL J., SCHMIDTOBREICK L., EDEROCLITE A., et al.
2022MNRAS.510.4180S 102       D         F     2 55 ~ Searching for nova shells around cataclysmic variables - II. A second campaign. SAHMAN D.I. and DHILLON V.S.
2022ApJ...928...20B viz 17       D               2 1219 10 New Variable Hot Subdwarf Stars Identified from Anomalous Gaia Flux Errors, Observed by TESS, and Classified via Fourier Diagnostics. BARLOW B.N., CORCORAN K.A., PARKER I.M., et al.
2022A&A...662A..40C viz 17       D               1 62976 9 The population of hot subdwarf stars studied with Gaia. IV. Catalogues of hot subluminous stars based on Gaia EDR3. CULPAN R., GEIER S., REINDL N., et al.
2023AJ....165..163C viz 17       D               1 1619 ~ Galactic Model Parameters and Spatial Density of Cataclysmic Variables in the Gaia Era: New Constraints on Population Models. CANBAY R., BILIR S., OZDONMEZ A., et al.
2023MNRAS.525.1953B 540       D S   X C F     10 47 ~ TESS light curves of cataclysmic variables - III - More superhump systems among old novae and nova-like variables. BRUCH A.
2024A&A...686A..25D viz 18       D               1 401 ~ A 500 pc volume-limited sample of hot subluminous stars I. Space density, scale height, and population properties. DAWSON H., GEIER S., HEBER U., et al.
2025A&A...693A.268R viz 19       D               1 581 ~ Variability in hot sub-luminous stars and binaries: Machine-learning analysis of Gaia DR3 multi-epoch photometry. RANAIVOMANANA P., UZUNDAG M., JOHNSTON C., et al.
2024ApJ...977..153B 959       D S   X C       20 123 ~ The AH Pictoris Syndrome: Continuous Trains of Stunted Outbursts in Novalike Variables. BRUCH A.
2025ApJS..277...29H 905       D S   X         19 64 ~ Stunted Outbursts and Z Cam-like Behaviors in the Long-term Light Curves of Novalike Cataclysmic Variables. HONEYCUTT R.K., ROBERTSON J.W. and RADZOM B.T.
2025ApJ...993...34D 19       D               1 57 ~ Hunt for the mHz Variability in TESS and XMM-Newton Observations of Nova-like Cataclysmic Variables. DOBROTKA A., MAGDOLEN J. and MELICHERCIK M.

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