Search Results - "Pit, Nikolaj V."
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Discovery of standstills in the SU UMa-type dwarf nova NY Serpentis
Published in Publications of the Astronomical Society of Japan (01-04-2019)“…Abstract We found that the SU UMa-type dwarf nova NY Ser in the period gap [orbital period 0.097558(6) d] showed standstills twice in 2018. This is the first…”
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First detection of two superoutbursts during the rebrightening phase of a WZ Sge-type dwarf nova: TCP J21040470+4631129
Published in Publications of the Astronomical Society of Japan (01-06-2020)“…Abstract We report on photometric and spectroscopic observations and analysis of the 2019 superoutburst of TCP J21040470+4631129. This object showed a 9 mag…”
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3
Survey of period variations of superhumps in SU UMa-type dwarf novae. X. The tenth year (2017)
Published in Publications of the Astronomical Society of Japan (01-02-2020)“…Abstract Continuing the project described by Kato et al. (2009, PASJ, 61, S395), we collected times of superhump maxima for 102 SU UMa-type dwarf novae…”
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4
Spectroscopic and photometric observations of dwarf nova superoutbursts by the 3.8 m telescope Seimei and the Variable Star Network
Published in Publications of the Astronomical Society of Japan (01-06-2021)“…Abstract We present spectroscopic and photometric observations of 17 dwarf-nova superoutbursts obtained by KOOLS-IFU mounted on the 3.8 m telescope Seimei at…”
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5
NY Serpentis: SU UMa-type nova in the period gap with diversity of normal outbursts
Published in Publications of the Astronomical Society of Japan (01-12-2014)“…Abstract We present a photometric study of NY Ser, an in-the-gap SU UMa-type nova, in 2002 and 2013. We determined the duration of its superoutburst and the…”
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6
Analysis of the IW And star ASAS J071404+7004.3
Published 23-02-2022“…We made a time-resolved photometric campaign of the bright cataclysmic variable ASAS J071404+7004.3 in 2020. Inight et al. (2022, arXiv/2109.14514) recently…”
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Spectroscopic and Photometric Observations of Dwarf Nova Superoutbursts by the 3.8 m Telescope Seimei and the Variable Star Network
Published 11-04-2021“…We present spectroscopic and photometric observations of 17 dwarf-nova superoutbursts obtained by KOOLS-IFU mounted on the 3.8 m telescope Seimei at Okayama…”
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8
First Detection of Two Superoutbursts during Rebrightening Phase of a WZ Sge-type Dwarf Nova: TCP J21040470+4631129
Published 22-04-2020“…We report photometric and spectroscopic observations and analysis of the 2019 superoutburst of TCP J21040470+4631129. This object showed a 9-mag superoutburst…”
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9
Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae. X: The Tenth Year (2017)
Published 25-12-2019“…Continuing the project described by Kato et al. (2009, PASJ, 61, S395, arXiv/0905.1757), we collected times of superhump maxima for 102 SU UMa-type dwarf novae…”
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10
Discovery of Standstills in the SU UMa-Type Dwarf Nova NY Serpentis
Published 16-01-2019“…We found that the SU UMa-type dwarf nova NY Ser in the period gap [orbital period 0.097558(6) d] showed standstills twice in 2018. This is the first clear…”
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Journal Article -
11
Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae. IX: The Ninth Year (2016-2017)
Published 30-06-2017“…Continuing the project described by Kato et al. (2009, arXiv:0905.1757), we collected times of superhump maxima for 127 SU UMa-type dwarf novae observed mainly…”
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12
Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae. VIII: The Eighth Year (2015-2016)
Published 20-05-2016“…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…”
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13
NY Serpentis: SU UMa-Type Nova in the Period Gap with Diversity of Normal Outbursts
Published 19-08-2014“…We present photometric study of NY Ser, an in-the-gap SU UMa-type nova, in 2002 and 2013. We determined the duration of the superoutburst and the mean…”
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Journal Article -
14
Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae. VII: The Seventh Year (2014-2015)
Published 20-07-2015“…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…”
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