March 2022 - vsnet-newvar - ooruri.kusastro.kyoto-u.ac.jp

[vsnet-newvar 9110] BMAM-V547: VY Scl star currently in low state
by Taichi Kato 14 Mar '22

14 Mar '22

BMAM-V547: VY Scl star currently in low state ASAS-SN data: https://asas-sn.osu.edu/sky-patrol/coordinate/1c81a2ee-0aa0-4a8d-a4c0-b8d07…

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[vsnet-newvar 9109] BMAM-V625: IW And+E
by Taichi Kato 14 Mar '22

14 Mar '22

BMAM-V625: IW And+E From ZTF data. Heartbeat state in 2018. Long standstill in 2019.

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[vsnet-newvar 9108] BMAM-V546: VY Scl+E
by Taichi Kato 14 Mar '22

14 Mar '22

BMAM-V546: VY Scl+E From ZTF data. Low state in late 2021 fainter than 21 mag.

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[vsnet-newvar 9107] PTF09o: polar
by Taichi Kato 14 Mar '22

14 Mar '22

PTF09gk: polar From ZTF data. Porb=0.0603462(1) d. Single pole. Nearly sinusoidal. Low state in 2018.

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[vsnet-newvar 9106] PTF09gk: polar
by Taichi Kato 14 Mar '22

14 Mar '22

PTF09gk: polar From ZTF data. Porb=0.0603462(1) d. Single pole. Nearly sinusoidal. Low state in 2018.

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[vsnet-newvar 9105] ASASSN-21mh: SU UMa star
by Taichi Kato 14 Mar '22

14 Mar '22

ASASSN-21mh: SU UMa star Superoutbursts in the ZTF data. Time-resolved ZTF data on 2020 July 13 detected superhumps. The superhump period was near 0.06 d.

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[vsnet-newvar 9104] ASASSN-17eg: refined period and about type
by Taichi Kato 14 Mar '22

14 Mar '22

ASASSN-17eg: refined period and about type Using the ZTF data, I obtained a refined orbital period of 0.07859690(5) d. The mean light curve is unlike that of an short-period dwarf nova or novalike, but is a smooth sinusoidal one with a full amplitude of 0.26 mag. The object looks like to me basically a reflection variable. The 2019 outburst likely came from an accretion disk formed by a small amount of mass-transfer. The transverse velocity is twice larger than that of OV Boo and ASASSN-17eg is probably a population II binary.

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[vsnet-newvar 9103] CSS J062450.1+503114: superhump period
by Taichi Kato 13 Mar '22

13 Mar '22

CSS J062450.1+503114: superhump period Itoh-san and Josch Hambsch have reported observations. Well-defined superhumps have been observed and the period has been established to be 0.07768(2) d. The mean amplitude is 0.19 mag.

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[vsnet-newvar 9102] WFI J161953.3+031909: genuine eclipsing Z Cam (+SU UMa?) star in the period gap
by Taichi Kato 13 Mar '22

13 Mar '22

WFI J161953.3+031909: genuine eclipsing Z Cam (+SU UMa?) star in the period gap ZTF data indicate that this object is a genuine Z Cam star. Long standstill in 2021 Feb.-Sep. There has been no indication of the IW And-type phenomenon. Long outbursts in 2019 may have been superoutbursts. The supercycle(?) was 70-90 d with a long duty cycle. This would be classified as UGZ+UGSU(ER):+E.

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[vsnet-newvar 9100] CRTS J094327.3-272039 superoutburst
by Taichi Kato 11 Mar '22

11 Mar '22

CRTS J094327.3-272039 superoutburst YYYYMMDD(UT) mag observer 20211231.7147 <165C (Masayuki Moriyama) 20220210.5993 <164C (Masayuki Moriyama) 20220306.6399 13.66C (Masayuki Moriyama) 20220309.6518 13.92C (Masayuki Moriyama)

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