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

[vsnet-chat 8960] V404 Sct: Mira
by Taichi Kato 15 Oct '21

15 Oct '21

V404 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.

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[vsnet-chat 8959] V403 Sct: Mira
by Taichi Kato 15 Oct '21

15 Oct '21

V403 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.

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[vsnet-chat 8958] V401 Sct: Mira
by Taichi Kato 15 Oct '21

15 Oct '21

V401 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.

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[vsnet-chat 8957] V400 Sct: Mira/SR
by Taichi Kato 15 Oct '21

15 Oct '21

V400 Sct: Mira/SR https://arxiv.org/pdf/2110.07229.pdf ZTF data clearly show Mira/SR-type variation with an amplitude about 2 mag. The original period appears correct.

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[vsnet-chat 8956] V399 Sct: Mira/SR
by Taichi Kato 15 Oct '21

15 Oct '21

V399 Sct: Mira/SR https://arxiv.org/pdf/2110.07229.pdf ZTF data clearly show Mira/SR-type variation with an amplitude more than 2 mag. The original period appears correct.

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[vsnet-chat 8955] V398 Sct: Mira
by Taichi Kato 15 Oct '21

15 Oct '21

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.

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[vsnet-chat 8954] V397 Sct: Mira
by Taichi Kato 15 Oct '21

15 Oct '21

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.

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[vsnet-chat 8953] V394 Sct: Mira
by Taichi Kato 15 Oct '21

15 Oct '21

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.

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[vsnet-chat 8952] V392 Sct: Mira
by Taichi Kato 15 Oct '21

15 Oct '21

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.

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[vsnet-chat 8951] V388 Sct: Mira
by Taichi Kato 15 Oct '21

15 Oct '21

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.

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