The Eruptive Nature of the Variable Star CzeV195
Abstract CzeV195 is a variable star discovered by Jaroslav Trnka (CzeV) in 2017 and classified at the Variable Star Index as a suspected EA-type variable star. The SSV-UAI-GRAV research section of the Unione Astrofili Italiani, undertook an observing campaign with ground-based telescopes in 2024 June and July. The star turned out to be an eclipsing variable of the EA type with a period of 0.604905 days. It was possible to detect an oscillation between the primary and secondary minima, typical of chromospherically active stars such as BY Draconis. Thanks to Zwicky Transient Facility and All-Sky Automated Survey for Supernovae photometry, ourbursts typical of UV Cet eruptive stars were detected. Czev195 was ultimately classified after our studies as an EA+BY+UV.
Authors
- L. Strabla
- C. Lopresti (ORCID: https://orcid.org/0000-0003-0161-906X)
- S. Lora (ORCID: https://orcid.org/0000-0003-1027-9853)
- M. Barbieri (ORCID: https://orcid.org/0009-0001-0508-8959)
- U. Quadri
- L. Barbieri
- Ivo Peretto (ORCID: https://orcid.org/0000-0003-3833-2695)
- Lorenzo Sassaro (ORCID: https://orcid.org/0009-0002-4205-8633)
- Giovanni Furlato (ORCID: https://orcid.org/0009-0008-9086-3702)
- Paolo Madurini
Publication Details
- Journal
- Research Notes of the AAS
- Published
- 2025-02-18
- DOI
- https://doi.org/10.3847/2515-5172/adb611
- Primary Topic
- Stellar, planetary, and galactic studies
- Type
- article
- Field-Weighted Citation Impact
- 0.00