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| HS 0220+0603 , the SIMBAD biblio (32 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST11:19:41 |
| 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. | |||
|
2011A&A...527A.126P |
15 | D | 1 | 16772 | 65 | Cross-correlation of the 2XMMi catalogue with Data Release 7 of the Sloan Digital Sky Survey. | PINEAU F.-X., MOTCH C., CARRERA F., et al. | ||
| 2012MNRAS.422.2332R | 76 | X | 2 | 20 | 11 | The fight for accretion: discovery of intermittent mass transfer in BB Doradus in the low state. | RODRIGUEZ-GIL P., SCHMIDTOBREICK L., LONG K.S., et al. | ||
| 2012MmSAI..83..602R | 229 | K | X C | 5 | 12 | 5 | The low states of CVs at the upper edge of the period gap. | RODRIGUEZ-GIL P., SCHMIDTOBREICK L., LONG K.S., et al. | |
| 2015MNRAS.452..146R | 2106 | K A | D | X C | 54 | 19 | 9 | Dynamical masses of a nova-like variable on the edge of the period gap. | RODRIGUEZ-GIL P., SHAHBAZ T., MARSH T.R., et al. |
|
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. | ||
| 2016MNRAS.455L..16S | 54 | X | 1 | 3 | 91 | Three in one go: consequential angular momentum loss can solve major problems of CV evolution. | SCHREIBER M.R., ZOROTOVIC M. and WIJNEN T.P.G. | ||
| 2016AJ....152...27K | 39 | X | 1 | 3 | 3 | The new eclipsing CV MASTER OTJ192328.22+612413.5 - A possible SW Sextantis star. | KENNEDY M.R., CALLANAN P., GARNAVICH P.M., et al. | ||
| 2018AJ....156..198H | 16 | D | 1 | 26 | ~ | On the MV-inclination relationship for Nova-like variables. | HOWELL S.B. and MASON E. | ||
|
2018AJ....156..231W |
40 | X | 1 | 6 | ~ | An optical study of two VY Sculptoris-type cataclysmic binary stars: V704 And and RX J2338+431. | WEIL K.E., THORSTENSEN J.R. and HABERL F. | ||
|
2019MNRAS.486.5535M |
138 | D | X | 4 | 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...43H |
16 | D | 2 | 182 | 17 | Spectroscopically identified cataclysmic variables from the LAMOST survey. I. The sample. | HOU W., LUO A.-L., LI Y.-B., 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. | ||
| 2020MNRAS.494..425R | 288 | X | 7 | 18 | ~ | When the disc's away, the stars will play: dynamical masses in the nova-like variable KR Aur with a pinch of accretion. | RODRIGUEZ-GIL P., SHAHBAZ T., TORRES M.A.P., et al. | ||
| 2021MNRAS.501.3046F | 17 | D | 1 | 9 | ~ | Will post-nova V1315 Aql enter into hibernation? | FANG X. and QIAN S. | ||
|
2021ApJ...914....5S |
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. | ||
|
2021ApJS..257...65S |
17 | D | 2 | 328 | 5 | A catalog of 323 cataclysmic variables from LAMOST DR6. | SUN Y., CHENG Z., YE S., et al. | ||
|
2022MNRAS.509.2674G |
17 | D | 2 | 3067 | 5 | White dwarfs identified in LAMOST Data Release 5. | GUO J., ZHAO J., ZHANG H., 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. | |
|
2023ApJS..264...17Z |
17 | D | 3 | 31380 | 1 | Stellar Parameters and Spectroscopic Properties of TESS Objects Observed in the LAMOST Low- and Medium-resolution Spectral Survey. | ZHANG L.-Y., SU T., MISRA P., et al. | ||
|
2023AJ....165..148H |
17 | D | 2 | 220 | 1 | Spectroscopically Identified Cataclysmic Variables from the LAMOST Survey. II. Period Estimates. | HOU W., LUO A.-L., DONG Y.-Q., 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. | ||||
| 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 | 421 | D | X C | 9 | 55 | ~ | TESS Light Curves of Cataclysmic Variables. IV. A Synoptic View of Eclipsing Old Novae and Novalike Variables. | BRUCH A. | |
| 2024A&A...690A.218A | 90 | X | 2 | 30 | ~ | The mass of the white dwarf in YY Dra (=DO Dra): Dynamical measurement and comparative study with X-ray estimates. | ALVAREZ-HERNANDEZ A., TORRES M.A.P., SHAHBAZ T., et al. | ||
| 2025ApJ...984....9Z | 19 | D | 1 | 108 | ~ | Searching for Accreting Compact Binary Systems from Spectroscopy and Photometry: Application to LAMOST Spectra. | ZHAO X., WANG S. and LIU J. | ||
| 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. |