Detection of Contact Binary Candidates Observed By TESS Using the Autoencoder Neural Network

Detection of Contact Binary Candidates Observed By TESS Using the Autoencoder Neural Network

A contact binary may be the progenitor of a red nova that eventually produces a merger event and have a cut-off period of around 0.2 days. Therefore, a large number of contact binaries is needed to search for the progenitor of red novae and to study the characteristics of short-period contact binari...

Πλήρης περιγραφή

Λεπτομέρειες βιβλιογραφικής εγγραφής
Κύριοι συγγραφείς:	Xu Ding, ZhiMing Song, ChuanJun Wang, KaiFan Ji
Μορφή:	Άρθρο
Γλώσσα:	English
Έκδοση:	IOP Publishing 2024-01-01
Σειρά:	The Astronomical Journal
Θέματα:	Binary stars Eclipsing binary stars Contact binary stars
Διαθέσιμο Online:	https://doi.org/10.3847/1538-3881/ad3048

Παρόμοια τεκμήρια

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A Possible Explanation of W-type Phenomena in V694 Peg
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KIC 9028474: A Long-period Eclipsing Binary on a Highly Eccentric Orbit
ανά: Orkun Özdarcan
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The ELM Survey South. II. Two Dozen New Low-mass White Dwarf Binaries
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Photometric and Spectroscopic Investigations of Three Large Amplitude Contact Binaries
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Investigating Period Variability Mechanisms in Eclipsing Binary Stars through Eclipsing Time Variation Analysis: A Case Study of TZ Bootis
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ανά: R. Pazhouhesh, κ.ά.
Έκδοση: (2017-03-01)

The Evolutionary Statuses of Solar Type Detached Eclipsing Binary Stars
ανά: Chanisa Kanjanascul, κ.ά.
Έκδοση: (2012-06-01)

Orbital Decay in an Accreting and Eclipsing 13.7 Minute Orbital Period Binary with a Luminous Donor
ανά: Kevin B. Burdge, κ.ά.
Έκδοση: (2023-01-01)

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FX UMa: A New Heartbeat Binary System with Linear and Nonlinear Tidal Oscillations and δ Sct Pulsations
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An Estimate of the Binary Star Fraction among Young Stars at the Galactic Center: Possible Evidence of a Radial Dependence
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Evidence for a Close-in Tertiary Orbiting around the Algol-type System HZ Dra with Tidal Splitting and Spots Activities
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