- vsnet-newvar - ooruri.kusastro.kyoto-u.ac.jp

[vsnet-newvar 9228] Gaia19dhy: most likely AM CVn-type dwarf nova
by Taichi Kato 09 Apr '22

09 Apr '22

Gaia19dhy: most likely AM CVn-type dwarf nova From ZTF data. Short superoutburst, long dip, followed by rebrightenings. Long bright state continued.

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[vsnet-newvar 9227] Gaia19dnv: eclipsing polar
by Taichi Kato 09 Apr '22

09 Apr '22

Gaia19dnv: eclipsing polar From ZTF data. Porb=0.0694359(2) d. Eclipse near the peak. Minimum of eclipse below the detection limit.

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[vsnet-newvar 9226] Gaia19dvf: most likely WZ Sge star
by Taichi Kato 09 Apr '22

09 Apr '22

Gaia19dvf: most likely WZ Sge star From ZTF data. Long rebrightening.

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[vsnet-newvar 9225] Gaia19dyt: most likely WZ Sge star
by Taichi Kato 09 Apr '22

09 Apr '22

Gaia19dyt: most likely WZ Sge star From ZTF data. Long rebrightening.

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[vsnet-newvar 9224] Gaia19eac: IW And star
by Taichi Kato 09 Apr '22

09 Apr '22

Gaia19eac: IW And star From ZTF data. Typical in 2019-2020.

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[vsnet-newvar 9223] Gaia20ded: possible AM CVn-type dwarf nova
by Taichi Kato 09 Apr '22

09 Apr '22

Gaia20ded: possible AM CVn-type dwarf nova From ZTF data. Short superoutburst, dip, rebrightening followed by long rebrightening.

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[vsnet-newvar 9222] Gaia20dlu: polar
by Taichi Kato 09 Apr '22

09 Apr '22

Gaia20dlu: polar From ZTF data. Porb=0.1009896(2) d. Single maximum per cycle.

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[vsnet-newvar 9221] Gaia20ecp: likely WZ Sge star with multiple rebrightenings
by Taichi Kato 09 Apr '22

09 Apr '22

Gaia20ecp: likely WZ Sge star with multiple rebrightenings From ZTF data. At least five rebrightenings.

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[vsnet-newvar 9220] Gaia20eio: polar
by Taichi Kato 09 Apr '22

09 Apr '22

Gaia20eio: polar From ZTF data. Porb=0.0621926(1) d. Double-peaked maximum. X-ray: 190051.4 +405008 (2000.0) 1RXS-F_J190051.5+405009 0.028 -0.67 0.81

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[vsnet-newvar 9219] ASASSN-22eb: new SU UMa-type dwarf nova
by Taichi Kato 08 Apr '22

08 Apr '22

ASASSN-22eb: new SU UMa-type dwarf nova Josch Hambsch and Itoh-san have reported observations. Hambsch's data on Apr. 7 showed clear superhumps. The period was about 0.055 d. This object could be a WZ Sge star.

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