LAMOST J171013+532646: A detached short-period noneclipsing hot subdwarf + white dwarf binary

pc \), with a Gaia G-band magnitude of 12.59. This renders it conducive for continuous observations. The spectral temperature is around 25164 K, in agreement with fitting results K \)) based on a spectral energy distribution. The TESS light curve displays ellipsoidal variation and Doppler beaming without eclipsing features. Through fitting the TESS light curve using the Wilson-Devinney code, we determined the masses for the sdB (\(M_1 = odot \)) and the compact object (\(M_2 = odot \)); the compact object likely is a WD. Furthermore, MESA models suggest that the sdB, with a helium core mass of 0.431 odot \) and a hydrogen envelope mass of \(1.3 odot \), is in the early helium main-sequence phase. The MESA binary evolution shows that the J1710 system is expected to evolve into a double WD system. This means that it is an important source of low-frequency gravitational waves.

Authors

Institutions

Publication Details

Journal
Astronomy and Astrophysics
Published
2024-12-18
DOI
https://doi.org/10.1051/0004-6361/202451415
Citations
3
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
0.99
Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

LAMOST J171013+532646: A detached short-period noneclipsing hot subdwarf + white dwarf binary

Haotong Zhang, Yao Cheng, Hailong Yuan, Zhongrui Bai et al.
3 citations
Astronomy and Astrophysics
Stellar, planetary, and galactic studies
0.99
article

LAMOST J171013+532646: A detached short-period noneclipsing hot subdwarf + white dwarf binary

Haotong Zhang, Yao Cheng, Hailong Yuan, Zhongrui Bai, Junfeng Wang, Yuji He, Mingkuan Yang, Zhenwei Li, Xuefei Chen, Yiqiao Dong, X. T. Huang, Mengxin 梦欣 Wang 汪
article en
3 citations

Abstract

pc \), with a Gaia G-band magnitude of 12.59. This renders it conducive for continuous observations. The spectral temperature is around 25164 K, in agreement with fitting results K \)) based on a spectral energy distribution. The TESS light curve displays ellipsoidal variation and Doppler beaming without eclipsing features. Through fitting the TESS light curve using the Wilson-Devinney code, we determined the masses for the sdB (\(M_1 = odot \)) and the compact object (\(M_2 = odot \)); the compact object likely is a WD. Furthermore, MESA models suggest that the sdB, with a helium core mass of 0.431 odot \) and a hydrogen envelope mass of \(1.3 odot \), is in the early helium main-sequence phase. The MESA binary evolution shows that the J1710 system is expected to evolve into a double WD system. This means that it is an important source of low-frequency gravitational waves.

Astronomy and Astrophysics
Xiamen University (CN), Chinese Academy of Sciences (CN), Yunnan Observatories (CN), National Astronomical Observatories (CN), University of Chinese Academy of Sciences (CN), Xiamen University of Technology (CN)
Affordable and clean energy
Openalex Percentile: Top 22%
Stellar, planetary, and galactic studies
0.99
DOIOpen Access PDFOpenAlex
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.

LAMOST J171013+532646: A detached short-period noneclipsing hot subdwarf + white dwarf binary — Haotong Zhang, Yao Cheng, et al. · Astronomy and Astrophysics (2024) | TGRS Research Map | TGRS