Periodic Variability of the Central Stars of Planetary Nebulae Surveyed through the Zwicky Transient Facility

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Hauptverfasser: Chen, Pinjian, Fang, Xuan, Chen, Xiaodian, Liu, Jifeng
Format: Preprint
Veröffentlicht: 2025
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author Chen, Pinjian
Fang, Xuan
Chen, Xiaodian
Liu, Jifeng
author_facet Chen, Pinjian
Fang, Xuan
Chen, Xiaodian
Liu, Jifeng
contents A consensus has been reached in recent years that binarity plays an important role in the formation and evolution of a significant fraction of planetary nebulae (PNe). Utilizing the archived photometric data from the Zwicky Transient Facility survey, we conducted a comprehensive data mining in search for brightness variations in a large sample of Galactic PNe. This effort leads to identification of 39 PNe, whose central stars exhibit periodic variation in light curves. Among these objects, 20 are known binary central stars of PNe, while the remaining 19 are new discoveries. Additionally, we identified 14 PNe with central stars displaying anomalous variation in light curves, as well as eight variables based on the high-cadence photometric data. Among the new discoveries of periodicity, we found compelling evidence of binary systems at the centres of two archetypal quadrupolar PNe. We also report on very peculiar brightness variation observed in the central core of the compact PN NGC6833. Several PNe in our sample deserve follow-up observations, both high-dispersion spectroscopy and high-precision photometry, to reveal the true nature of their central binarity or even multiplicity.
format Preprint
id arxiv_https___arxiv_org_abs_2501_06056
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Periodic Variability of the Central Stars of Planetary Nebulae Surveyed through the Zwicky Transient Facility
Chen, Pinjian
Fang, Xuan
Chen, Xiaodian
Liu, Jifeng
Solar and Stellar Astrophysics
Astrophysics of Galaxies
A consensus has been reached in recent years that binarity plays an important role in the formation and evolution of a significant fraction of planetary nebulae (PNe). Utilizing the archived photometric data from the Zwicky Transient Facility survey, we conducted a comprehensive data mining in search for brightness variations in a large sample of Galactic PNe. This effort leads to identification of 39 PNe, whose central stars exhibit periodic variation in light curves. Among these objects, 20 are known binary central stars of PNe, while the remaining 19 are new discoveries. Additionally, we identified 14 PNe with central stars displaying anomalous variation in light curves, as well as eight variables based on the high-cadence photometric data. Among the new discoveries of periodicity, we found compelling evidence of binary systems at the centres of two archetypal quadrupolar PNe. We also report on very peculiar brightness variation observed in the central core of the compact PN NGC6833. Several PNe in our sample deserve follow-up observations, both high-dispersion spectroscopy and high-precision photometry, to reveal the true nature of their central binarity or even multiplicity.
title Periodic Variability of the Central Stars of Planetary Nebulae Surveyed through the Zwicky Transient Facility
topic Solar and Stellar Astrophysics
Astrophysics of Galaxies
url https://arxiv.org/abs/2501.06056