Buchumschlag

Near-Contact Binaries on the Path to Contact Binaries

Fuente: arXiv

Gespeichert in:

Bibliographische Detailangaben
1. Verfasser:	Stȩpień, K.
Format:	Preprint
Veröffentlicht:	2026
Schlagworte:	Solar and Stellar Astrophysics
Online-Zugang:	Acceder al recurso
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!

Ähnliche Einträge

Searching for Contact Binaries with LAMOST and TESS
von: Wu, Ting, et al.
Veröffentlicht: (2026)

Exploring Contact Binaries: Observational Analysis of four W Uma Binaries Using Photometry and Spectroscopy
von: Panchal, Alaxender, et al.
Veröffentlicht: (2025)

Photometric and Spectroscopic Investigations of Three Large Amplitude Contact Binaries
von: Xu, Xin, et al.
Veröffentlicht: (2024)

Fundamental Parameters for Totally Eclipsing Contact Binaries Observed by TESS
von: Ding, Xu, et al.
Veröffentlicht: (2025)

Photometric Analysis of 30 Contact Binaries in M31
von: Gao, Xiang, et al.
Veröffentlicht: (2025)

Binary Analysis and Period Study of the Long-Period, High Mass Ratio Contact Binary KIC 7766185
von: Larsen, Conor M, et al.
Veröffentlicht: (2025)

Optical Flares Detected on a Contact Binary: The First Photometric and Spectroscopic Analysis of a Long-period Low Mass Ratio Contact Binary HAT 307-0007476
von: Li, Ling-Zhi, et al.
Veröffentlicht: (2025)

The Critical Mass Ratio for W UMa-type Contact Binary Systems
von: Arbutina, Bojan, et al.
Veröffentlicht: (2024)

V717 Andromedae: An Active Low Mass Ratio Contact Binary
von: Wadhwa, S. S., et al.
Veröffentlicht: (2025)

Period Changes of 14,127 Contact Eclipsing Binaries in the Galactic Bulge
von: Hong, Kyeongsoo, et al.
Veröffentlicht: (2022)

Physical Parameters of 146 Contact Binaries Derived from Light and Radial Velocity Curves
von: Li, Kai, et al.
Veröffentlicht: (2026)

The First Photometric Analysis of Two Low Mass Ratio Contact Binary Systems In TESS Survey
von: Cheng, Qiyuan, et al.
Veröffentlicht: (2024)

BSN-III: The First Multiband Photometric Study on the Eight Total Eclipse Contact Binary Stars
von: Poro, Atila, et al.
Veröffentlicht: (2025)

Reanalyzing the Light Curves and Absolute Parameters of Twenty Contact Binary Stars Using TESS Data
von: Paki, Ehsan, et al.
Veröffentlicht: (2024)

BSN: Light Curve Modeling and Orbital Evolution of the Total-Eclipse Contact Binary EZ Oct
von: Ababafi, Asma, et al.
Veröffentlicht: (2025)

Minute-cadence Observations of the LAMOST Fields with the TMTS: VI. Absolute Physical Parameters of Contact Binaries
von: Xia, Qiqi, et al.
Veröffentlicht: (2024)

BSN: First Light Curve Study of the Low Mass Contact Binary V0610 Vir
von: Alizadehsabegh, Ailar, et al.
Veröffentlicht: (2023)

BSN: The First Photometric Analysis of Contact Binary Systems V1961 Cyg and V0890 Lyr
von: Baudart, Sabrina, et al.
Veröffentlicht: (2024)

The BSN Application-I: Photometric Light Curve Solutions of Contact Binary Systems
von: Paki, Ehsan, et al.
Veröffentlicht: (2025)

Detection of Contact Binary Candidates Observed By TESS Using Autoencoder Neural Network
von: Ding, Xu, et al.
Veröffentlicht: (2024)

Period-Luminosity-Metallicity-Color Relations of Late-type Contact Binaries in the Big Data Era
von: Song, Lian-Yun, et al.
Veröffentlicht: (2024)

BSN-IV: The First Multiband Light Curve Study of Five W UMa-type Contact Binary Systems
von: Poro, Atila, et al.
Veröffentlicht: (2025)

BSN: The First Multiband Light Curve Analysis of the W UMa-type Contact Binary System EM Tucanae
von: Houshiar, Sepideh, et al.
Veröffentlicht: (2025)

BSN: Photometric Light Curve Analysis of Two Contact Binary Systems LS Del and V997 Cyg
von: Poro, Atila, et al.
Veröffentlicht: (2024)

Detailed TESS-Based Light Curve Modeling and Fundamental Parameter Estimation of 27 W UMa-Type Contact Binaries
von: Poro, Atila, et al.
Veröffentlicht: (2026)

BSN-II: The First Light Curve Study of Eight Total Eclipsing Contact Binary Stars with Shallow Fillout Factors
von: Poro, Atila, et al.
Veröffentlicht: (2025)

First Light Curve Analysis of NSVS 8294044, V1023 Her, and V1397 Her Contact Binary Systems
von: Poro, Atila, et al.
Veröffentlicht: (2024)

Four Total Eclipsing Contact Binary Systems: The First Photometric Light Curve Solutions Employing TESS and Gaia Surveys
von: Poro, Atila, et al.
Veröffentlicht: (2025)

Photometric and Spectroscopic Studies of Four Low Mass-ratio Contact Binaries with Period Longer than 0.7 days
von: Wang, Yi-Fan, et al.
Veröffentlicht: (2025)

Low Mass Contact Binaries: Orbital Stability at Extreme Low Mass Ratios
von: Wadhwa, Surjit S., et al.
Veröffentlicht: (2024)

Detailed Investigation of a W UMa Contact Binary with an Ultralow Mass Ratio and a Third-Body as a Potential Merger Candidate
von: Poro, Atila, et al.
Veröffentlicht: (2026)

BSN: First Photometric Light Curve Analysis of Two W-type Contact Binary Systems OP Boo and V0511 Cam
von: Poro, Atila, et al.
Veröffentlicht: (2024)

W UMa-Type Contact Binaries in the Tidal Tails of Young Open Cluster COIN-Gaia 25 and Mamajek 4
von: Bin, Xiang, et al.
Veröffentlicht: (2026)

Physical Parameters of 11,100 Short-Period ASAS-SN Eclipsing Contact Binaries
von: Li, Xu-Zhi, et al.
Veröffentlicht: (2024)

BSN-V: The First Detailed Light Curve Modeling of Eight Totally Eclipsing Contact Binary Stars Using Ground-Based and TESS Observations
von: Poro, Atila, et al.
Veröffentlicht: (2025)

BSN-VI: Multiband Light Curve Modeling of Four W UMa-Type Contact Binaries I. Revisiting Energy Transfer Mechanisms and Luminosity Behavior
von: Sarvari, Elham, et al.
Veröffentlicht: (2026)

A Low Metallicity Massive Contact Binary Star System Candidate in WLM identified by Hubble and James Webb Space Telescope imaging
von: Gull, Maude, et al.
Veröffentlicht: (2024)

Extremely Low Mass Ratio Contact Binaries. II. The First Photometric and Spectroscopic Investigations of Six Systems with Orbital Periods Longer than 0.5 days
von: Liu, Fei, et al.
Veröffentlicht: (2025)

Photometric and Spectroscopic study of Ten Low Mass Ratio Contact Binary Systems: Orbital Stability, O'Connell Effect and Infra-red Calcium Line Filling
von: Wadhwa, Surjit S., et al.
Veröffentlicht: (2024)

Spectroscopic and Decade-long Photometric Observations of the Contact Binary V2790 Ori: Evidence for a Brown Dwarf Companion and a Solar-like Magnetic Activity Cycle
von: Wang, Si-Rui, et al.
Veröffentlicht: (2025)