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| HS 0455+8315 , the SIMBAD biblio (20 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST21:50:13 |
| 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 |
1714 | 277 | A catalog and atlas of cataclysmic variables: the living edition. | DOWNES R.A., WEBBINK R.F., SHARA M.M., et al. | |||||
| 2005ASPC..330..335R | 7 | 7 | The role of the SW Sextantis stars in the picture of CV evolution. | RODRIGUEZ-GIL P. | |||||
| 2007MNRAS.377.1747R | 1112 | A | D | S X C F | 28 | 52 | 78 | SW Sextantis stars: the dominant population of cataclysmic variables with orbital periods between 3 and 4h. | RODRIGUEZ-GIL P., GANSICKE B.T., HAGEN H.-J., et al. |
|
2008NewA...13..133A |
15 | D | 459 | 29 | Spatial distribution and galactic model parameters of cataclysmic variables. | AK T., BILIR S., AK S., et al. | |||
| 2011NewA...16...19S | 15 | D | 1 | 26 | 1 | Two new systems with enhanced UV line flux ratios as indication of the evolution of cataclysmic variables. | SANAD M.R. | ||
|
2015A&A...584A..40K |
78 | X | 2 | 28 | 3 | 2MASS J22560844+5954299: the newly discovered cataclysmic star with the deepest eclipse. | KJURKCHIEVA D., KHRUZINA T., DIMITROV D., et al. | ||
|
2020MNRAS.492L..40A |
16 | D | 1 | 1220 | 31 | Disentangling cataclysmic variables in Gaia's HR diagram. | ABRIL J., SCHMIDTOBREICK L., EDEROCLITE A., et al. | ||
| 2022MNRAS.509.2362L | 89 | F | 1 | 2 | 8 | Minute-cadence observations of the LAMOST fields with the TMTS: I. Methodology of detecting short-period variables and results from the first-year survey. | LIN J., WANG X., MO J., et al. | ||
|
2022ApJS..258...16P |
17 | D | 1 | 4582 | 43 | TESS Eclipsing Binary stars. I. Short-cadence observations of 4584 eclipsing binaries in sectors 1-26. | PRSA A., KOCHOSKA A., CONROY K.E., 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. | |
|
2022A&A...662A..40C |
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 |
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. | ||
| 2023JAVSO..51...74B | O | 18 | ~ | Long-term Study of Changes in the Orbital Periods of 18 Eclipsing SW Sextantis Stars. | BOYD D. | ||||
| 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. | |
| 2024ApJ...966..155S | 108 | D | X | 3 | 54 | ~ | Evolutionary Period Changes for 52 Cataclysmic Variables, and the Failure for the Most-fundamental Prediction of the Magnetic Braking Model. | SCHAEFER B.E. | |
| 2024ApJS..273....6B | 511 | D | X | 12 | 55 | ~ | TESS Light Curves of Cataclysmic Variables. IV. A Synoptic View of Eclipsing Old Novae and Novalike Variables. | BRUCH A. | |
|
2025A&A...693A.268R |
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. | ||
| 2025ApJS..277...29H | 485 | D | S X | 10 | 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...988...35S | 19 | D | 1 | 85 | ~ | Evolutionary Period Changes for 25 X-Ray Binaries and the Measurement of an Empirical Universal Law for Angular Momentum Loss in Accreting Binaries. | SCHAEFER B.E. | ||
| 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. |