ZTF J172132.75+445851.0: A Possible New Cataclysmic Variable of the VY Sculptoris Type

Fuente: arXiv
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Autores principales: Bernhard, Klaus, Lloyd, Christopher, Frank, Peter, Moschner, Wolfgang
Formato: Preprint
Publicado: 2025
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author Bernhard, Klaus
Lloyd, Christopher
Frank, Peter
Moschner, Wolfgang
author_facet Bernhard, Klaus
Lloyd, Christopher
Frank, Peter
Moschner, Wolfgang
contents We report the discovery of ZTF J172132.75+445851.0 as a new possible VY Sculptoris variable, with an orbital period of 0.109765426(44) days. Survey observations from 2005 to the present reveal significant activity in the system, with brightness variations ranging between 18.1 and 21.3 (zr) magnitudes, including deep fades exceeding an amplitude of 3 magnitudes.
format Preprint
id arxiv_https___arxiv_org_abs_2502_00736
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle ZTF J172132.75+445851.0: A Possible New Cataclysmic Variable of the VY Sculptoris Type
Bernhard, Klaus
Lloyd, Christopher
Frank, Peter
Moschner, Wolfgang
Solar and Stellar Astrophysics
We report the discovery of ZTF J172132.75+445851.0 as a new possible VY Sculptoris variable, with an orbital period of 0.109765426(44) days. Survey observations from 2005 to the present reveal significant activity in the system, with brightness variations ranging between 18.1 and 21.3 (zr) magnitudes, including deep fades exceeding an amplitude of 3 magnitudes.
title ZTF J172132.75+445851.0: A Possible New Cataclysmic Variable of the VY Sculptoris Type
topic Solar and Stellar Astrophysics
url https://arxiv.org/abs/2502.00736