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Periodic Variability of the Central Stars of Planetary Nebulae Surveyed through the Zwicky Transient Facility
Chen, Pinjian1,2; Fang, Xuan1,2,3,4; Chen, Xiaodian1,2,5; Liu, Jifeng1,2,5,6
2025-02-20
Source PublicationASTROPHYSICAL JOURNAL
ISSN0004-637X
Volume980Issue:2Pages:227
Contribution Rank3
AbstractA 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 of brightness variations in a large sample of Galactic PNe. This effort led 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 centers of two archetypal quadrupolar PNe. We also report on very peculiar brightness variation observed in the central core of the compact PN NGC 6833. 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.
DOI10.3847/1538-4357/ada94a
Indexed BySCI
Language英语
WOS KeywordBINARY CENTRAL STARS ; INFRARED-SURVEY-EXPLORER ; ABUNDANCE DISCREPANCY FACTORS ; WHITE-DWARF ; DOUBLE-DEGENERATE ; SPECTRAL-ANALYSIS ; COMMON ; DISCOVERY ; VELOCITY ; NUCLEUS
Funding ProjectYouth Talent Program[2021] ; Chinese Academy of Sciences (CAS, Beijing) ; National Natural Science Foundation of China (NSFC)[11988101] ; National Science Foundation[AST-1440341] ; National Science Foundation[AST-2034437] ; Oskar Klein Center at Stockholm University ; Drexel University
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:001424621900001
PublisherIOP Publishing Ltd
Funding OrganizationYouth Talent Program ; Chinese Academy of Sciences (CAS, Beijing) ; National Natural Science Foundation of China (NSFC) ; National Science Foundation ; Oskar Klein Center at Stockholm University ; Drexel University
Citation statistics
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/7446
Collection中国科学院新疆天文台
Corresponding AuthorFang, Xuan
Affiliation1.Chinese Acad Sci NAOC, CAS Key Lab Opt Astron, Natl Astron Observ, 20A Datun Rd, Beijing 100101, Peoples R China
2.Univ Chinese Acad Sci, Sch Astron & Space Sci, Beijing 100049, Peoples R China
3.Chinese Acad Sci, Xinjiang Astron Observ, 150 Sci 1-St, Urumqi 830011, Xinjiang, Peoples R China
4.Univ Hong Kong, Fac Sci, Lab Space Res, Pokfulam Rd, Hong Kong, Peoples R China
5.Beijing Normal Univ, Inst Frontiers Astron & Astrophys, Beijing 102206, Peoples R China
6.Chinese Acad Sci NAOC, New Cornerstone Sci Lab, Natl Astron Observ, Beijing 100101, Peoples R China
Corresponding Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Chen, Pinjian,Fang, Xuan,Chen, Xiaodian,et al. Periodic Variability of the Central Stars of Planetary Nebulae Surveyed through the Zwicky Transient Facility[J]. ASTROPHYSICAL JOURNAL,2025,980(2):227.
APA Chen, Pinjian,Fang, Xuan,Chen, Xiaodian,&Liu, Jifeng.(2025).Periodic Variability of the Central Stars of Planetary Nebulae Surveyed through the Zwicky Transient Facility.ASTROPHYSICAL JOURNAL,980(2),227.
MLA Chen, Pinjian,et al."Periodic Variability of the Central Stars of Planetary Nebulae Surveyed through the Zwicky Transient Facility".ASTROPHYSICAL JOURNAL 980.2(2025):227.
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