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20092026
most citedSurvey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae

194 citations · 683 across the 17 of their papers we have counts for

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astro-ph.SR2026

Photometric light curves analysis of SU UMa-type dwarf novae: the case of RZ LMi and KV Dra

I. B. Voloshina, A. N. Tarasenkov

The results of new photometric observations of two SU~UMa type dwarf novae are presented. Superhumps were detected on the light curves of these systems during superoutbursts and th…

astro-ph.SR2018★ 15 cited

DE CVn: an eclipsing post-common envelope binary with a circumbinary disk and a giant planet

Z. T Han, S. B. Qian, L. Y. Zhu +8

We present a timing analysis of the eclipsing post-common envelope binary (PCEB) DE CVn. Based on new CCD photometric observations and the published data, we found that the orbital…

astro-ph.SR2016★ 34 cited

Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae. VIII: The Eighth Year (2015-2016)

Taichi Kato, Franz-Josef Hambsch, Berto Monard +75

Continuing the project described by Kato et al. (2009, arXiv:0905.1757), we collected times of superhump maxima for 128 SU UMa-type dwarf novae observed mainly during the 2015-2016…

astro-ph.SR2015★ 51 cited

Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae. VII: The Seventh Year (2014-2015)

Taichi Kato, Franz-Josef Hambsch, Pavol A. Dubovsky +89

Continuing the project described by Kato et al. (2009, arXiv:0905.1757), we collected times of superhump maxima for 102 SU UMa-type dwarf novae observed mainly during the 2014-2015…

astro-ph.SR2014★ 50 cited

Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae. VI: The Sixth Year (2013-2014)

Taichi Kato, Pavol A. Dubovsky, Igor Kudzej +83

Continuing the project described by Kato et al. (2009, PASJ, 61, S395, arXiv:0905.1757), we collected times of superhump maxima for 56 SU UMa-type dwarf novae mainly observed durin…

astro-ph.SR2014★ 22 cited

Study of Negative and Positive Superhumps in ER Ursae Majoris

Tomohito Ohshima, Taichi Kato, Elena Pavlenko +45

We carried out the photometric observations of the SU UMa-type dwarf nova ER UMa during 2011 and 2012, which showed the existence of persistent negative superhumps even during the…

astro-ph.SR2013★ 54 cited

Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae. V: The Fifth Year (2012-2013)

Taichi Kato, Franz-Josef Hambsch, Hiroyuki Maehara +84

Continuing the project described by Kato et al. (2009a, arXiv:0905.1757), we collected times of superhump maxima for SU UMa-type dwarf novae mainly observed during the 2012-2013 se…

astro-ph.SR2012★ 79 cited

Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae. IV: The Fourth Year (2011-2012)

Taichi Kato, Franz-Josef Hambsch, Hiroyuki Maehara +85

Continuing the project described by Kato et al. (2009, arXiv:0905.1757), we studied 86 SU UMa-type dwarf novae. We confirmed the general trends such as the relation between period…

astro-ph.SR2011★ 59 cited

Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae. III: The Third Year (2010--2011)

Taichi Kato, Hiroyuki Maehara, Ian Miller +75

Continuing the project described by Kato et al. (2009, PASJ 61, S395, arXiv:0905.1757), we collected times of superhump maxima for 51 SU UMa-type dwarf novae mainly observed during…

astro-ph.SR2011★ 2 cited

MN Dra - In-the-Gap Dwarf Nova With Negative Superhumps

Elena Pavlenko, Taichi Kato, Max Andreev +9

The multi-site photometric observations of MN Dra were made over 77 nights in August-November, 2009. The total exposure was 433 hours. During this time the binary underwent two sup…

astro-ph.SR2010★ 101 cited

Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae. II: The Second Year (2009-2010)

Taichi Kato, Hiroyuki Maehara, Makoto Uemura +56

As an extension of the project in Kato et al. (2009, arXiv:0905.1757), we collected times of superhump maxima for 61 SU UMa-type dwarf novae mainly observed during the 2009-2010 se…

astro-ph.SR2010★ 6 cited

A long term spectroscopic and photometric study of the old nova HR Del

M. Friedjung, M. Dennefeld, I. Voloshina

The Nova HR Del, discovered in 1967, was found to be exceptionally bright in the optical and UV during the whole lifetime of the IUE satellite (ending in 1996) and appears to be st…

astro-ph.SR2009★ 194 cited

Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae

Taichi Kato, Akira Imada, Makoto Uemura +60

We systematically surveyed period variations of superhumps in SU UMa-type dwarf novae based on newly obtained data and past publications. In many systems, the evolution of superhum…