V398 Sct: Mira
https://arxiv.org/pdf/2110.07229.pdf
ZTF data clearly show Mira-type variation with
an amplitude more than 2.5 mag. The original period
appears correct.
V397 Sct: Mira
https://arxiv.org/pdf/2110.07229.pdf
ZTF data clearly show Mira-type variation with
an amplitude more than 4 mag. The original period
appears correct.
V394 Sct: Mira
https://arxiv.org/pdf/2110.07229.pdf
ZTF data clearly show Mira-type variation with
an amplitude more than 2.5 mag. The original period
appears correct.
V392 Sct: Mira
https://arxiv.org/pdf/2110.07229.pdf
ZTF data clearly show Mira-type variation with
an amplitude more than 2 mag. The period appears
to be around 500 d.
V388 Sct: Mira
https://arxiv.org/pdf/2110.07229.pdf
ZTF data clearly show Mira-type variation with
an amplitude more than 3.5 mag. The original period
appears correct.
V387 Sct: Mira
https://arxiv.org/pdf/2110.07229.pdf
ZTF data clearly show Mira-type variation with
an amplitude more than 2.5 mag. The original period
appears correct.
V384 Sct: Mira
https://arxiv.org/pdf/2110.07229.pdf
ZTF data clearly show Mira-type variation with
an amplitude more than 3.5 mag. The original period
appears correct.
V386 Sct: Mira
https://arxiv.org/pdf/2110.07229.pdf
ZTF data clearly show Mira-type variation with
an amplitude more than 4 mag. The original period
appears correct.
Following VSOLJ bulletin are now available at
http://vsolj.cetus-net.org/bulletin.html
No.82 2021 Oct.
Algol-type system RZ Cas: Times of primary minima by different methods
Shin-ya Narusawa and Kazuo Nagai
Seiichiro Kiyota, VSOLJ