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| V* V1108 Her , the SIMBAD biblio (36 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST06:37:08 |
| 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. | |||||
| 2004PASP..116.1117P | 15 | 10 | A new cataclysmic variable in Hercules. | PRICE A., GARY B., BEDIENT J., et al. | |||||
| 2004BAVSR..53..141L | O | 13 | 0 | Aktivitaten zwischen April und August 2004. | LANGE T. | ||||
| 2004IAUC.8363....1N | 2 | 1 | 6 | Unusual cataclysmic variable in Hercules. | NAKANO S., NAKAMURA Y., ITAGAKI K., et al. | ||||
| 2004IAUC.8367....3B | 1 | 0 | Unusual cataclysmic variable in Hercules. | BEDIENT J. and PITTICHOVA J. | |||||
| 2004IAUC.8369....2S | 1 | 0 | Unusual cataclysmic variable in Hercules. | SCHAEFER B.E. | |||||
| 2004IAUC.8374....3P | 2 | 0 | Unusual cataclysmic variable in Hercules. | PRICE A., JAMES R., HENDEN A., et al. | |||||
| 2004JAVSO..33R..84P | 2 | ~ | BZ UMa and var Her 04: keeping us up at night (paper). | PRICE A. | |||||
|
2006IBVS.5721....1K |
1754 | 36 | The 78th name-list of variable stars. | KAZAROVETS E.V., SAMUS N.N., DURLEVICH O.V., et al. | |||||
| 2006PASJ...58L..19I | 12 | 12 | Discovery of a promising candidate of WZ Sge-type dwarf novae, ASAS 160048-4846.2: evidence for double-peaked humps. | IMADA A. and MONARD L.A.G.B. | |||||
| 2006AJ....132.1989C | 111 | T K | 5 | 4 |
Spitzer Space Telescope observations of Var Her 04: possible detection of dust formation in a superoutbursting tremendous outburst amplitude dwarf nova. |
CIARDI D.R., WACHTER S., HOARD D.W., et al. | |||
| 2006MNRAS.373..484K | 180 | 322 | The donor stars of cataclysmic variables. | KNIGGE C. | |||||
| 2005JAVSO..33..160T | 3 | 0 | Campaign '04 : AAVSO observing campaigns in 2004. | TEMPLETON M. and PRICE A. | |||||
| 2005JAVSO..33..264W | 4 | 0 | Charge-coupled device (CCD). | WALKER G. | |||||
|
2008NewA...13..133A |
15 | D | 459 | 29 | Spatial distribution and galactic model parameters of cataclysmic variables. | AK T., BILIR S., AK S., et al. | |||
| 2007PASJ...59..929I | 11 | 9 | Infrared spectroscopy of short-period cataclysmic variables. | ISHIOKA R., SEKIGUCHI K. and MAEHARA H. | |||||
|
2009ApJS..184..138H |
15 | D | 2 | 20623 | 68 | XID II: statistical cross-association of ROSAT bright source catalog X-ray sources with 2MASS point source catalog near-infrared sources. | HAAKONSEN C.B. and RUTLEDGE R.E. | ||
| 2010PASJ...62..187U | 15 | D | 1 | 76 | 4 | Dwarf novae in the shortest orbital period regime. I A new short superhump period dwarf nova, OT J055717+683226. | UEMURA M., ARAI A., KATO T., et al. | ||
| 2010PASJ...62..613U | 15 | D | 1 | 150 | 14 | Dwarf novae in the shortest orbital period regime: II. WZ Sge stars as the missing population near the period minimum | UEMURA M., KATO T., NOGAMI D., et al. | ||
| 2009PASJ...61S.395K | 389 | D | S X C | 9 | 218 | 200 | Survey of period variations of superhumps in SU UMa-type dwarf novae. | KATO T., IMADA A., UEMURA M., et al. | |
|
2010CoSka..40...19C |
72 | 8 | Photometric investigation of V466 And - a new WZ Sge-type dwarf nova. | CHOCHOL D., KATYSHEVA N.A., SHUGAROV S.Yu., et al. | |||||
| 2012PASJ...64...21K | 15 | D | 1 | 106 | 61 | Survey of period variations of superhumps in SU UMa-type dwarf novae. III. The third year (2010-2011). | KATO T., MAEHARA H., MILLER I., et al. | ||
| 2008JBAA..118...95S | 11 | 3 | Photometry and astrometry of SS Leo Minoris during the 2006 October superoutburst. | SHEARS J., BOYD D., KRAJCI T., et al. | |||||
| 2011Ap.....54..483P | 1008 | T K A | X F | 25 | 13 | 4 |
Features of the orbital variability in the brightness of the WZ Sge type dwarf nova V1108 Her. |
PAVLENKO E.P., KATO T., ANTONYUK O.I., et al. | |
| 2013PASJ...65..117N | 15 | D | 1 | 56 | 17 | WZ Sge-type dwarf novae with multiple rebrightenings : MASTER OT J211258.65+242145.4 and MASTER OT J203749.39+552210.3. | NAKATA C., OHSHIMA T., KATO T., et al. | ||
| 2015PASJ...67..108K | 94 | D | X | 3 | 186 | 94 | WZ Sge-type dwarf novae. | KATO T. | |
|
2016MNRAS.460.2526O |
16 | D | 1 | 638 | 28 | Statistical analysis of properties of dwarf novae outbursts. | OTULAKOWSKA-HYPKA M., OLECH A. and PATTERSON J. | ||
| 2017MNRAS.466.2855P | 16 | D | 2 | 52 | 64 | Effective temperatures of cataclysmic-variable white dwarfs as a probe of their evolution. | PALA A.F., GANSICKE B.T., TOWNSLEY 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. | ||
| 2020MNRAS.494.3799P | 16 | D | 1 | 171 | 108 | A Volume-limited Sample of Cataclysmic Variables from Gaia DR2: Space Density and Population Properties. | PALA A.F., GANSICKE B.T., BREEDT E., et al. | ||
|
2021MNRAS.504.2420I |
17 | D | 1 | 453 | 18 | Towards a volumetric census of close white dwarf binaries - I. Reference samples. | INIGHT K., GANSICKE B.T., BREEDT E., et al. | ||
| 2022MNRAS.510.6110P | 485 | D | X F | 11 | 53 | 32 | Constraining the evolution of cataclysmic variables via the masses and accretion rates of their underlying white dwarfs. | PALA A.F., GANSICKE B.T., BELLONI D., 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. | ||
|
2024A&A...687A.305M |
18 | D | 2 | 192 | ~ | Cataclysmic variables around the period-bounce: An eROSITA-enhanced multiwavelength catalog. | MUNOZ-GIRALDO D., STELZER B. and SCHWOPE A. | ||
| 2025PASP..137g4201S | 112 | D | C | 2 | 103 | ~ | Cataclysmic Variables in Triples: Formation Models and New Discoveries. | SHARIAT C., EL-BADRY K., NAOZ S., et al. | |
| 2026A&A...707A..62M | 70 | D | X | 2 | 43 | ~ | eROSITA selection of new period-bounce cataclysmic variables First follow-up confirmation using TESS and SDSS. | MUNOZ-GIRALDO D., STELZER B., SCHWOPE A., et al. |