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20062026
most citedPopulation synthesis for symbiotic stars with white dwarf accretors

93 citations · 455 across the 53 of their papers we have counts for

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38 papers · 1 filter

astro-ph.SR2026

LISA Double White Dwarfs in Triple Systems

Zhijun Wang, Guoliang Lü, Chunhua Zhu +5

Double white dwarfs (DWDs) in the Laser Interferometer Space Antenna (LISA) band are major Galactic gravitational-wave sources, but many tight DWD progenitors may reside in hierarc…

astro-ph.SR2026

SN 2021pfs: A Type Ia Supernova Likely Affected by Progenitor Metallicity, as Revealed by Comparison with Its Twin Counterpart

Abdusamatjan Iskandar, Xiaofeng Wang, Ali Esamdin +16

We present extensive photometric and spectroscopic observations of the normal type Ia supernovae (SNe Ia) 2021pfs, which occurred in the Seyfert 2 galaxy NGC 5427 at a redshift 0.0…

astro-ph.SR2026

Mass distribution of neutron stars in binary systems

Zhe Hu, GuoLiang Lv, ChunHua Zhu +5

It is known that the mass distribution of the known neutron stars (NSs) exhibits a bimodal pattern. The origin of this distribution remains a subject of debate. We constructed a su…

astro-ph.SR2026★ 1 cited

Adiabatic Mass Loss In Binary Stars. VI. Massive Helium Binary Stars

Lifu Zhang, Hongwei Ge, Zhenwei Li +6

The stability of binary mass transfer is a critical problem for binary evolution. We systematically calculate the adiabatic mass-loss model for naked helium stars with masses rangi…

astro-ph.SR2026

Evolution of cataclysmic variables under different magnetic braking prescriptions

Bingyao Zhou, Chunhua Zhu, Guoliang Lü +3

Context. The evolution of cataclysmic variables (CVs) - interacting binaries where a low-mass donor transfers matter to a white dwarf via an accretion disk - is critically controll…

astro-ph.SR2025

Formation of the Dormant Black Holes with Luminous Companions from Binary or Triple Systems

Zhuowen Li, Xizhen Lu, Guoliang Lü +6

Recently, a class of dormant black hole binaries with luminous companions (dBH-LC) has been observed, such as BH1, BH2, and BH3. Unlike previously discovered X-ray BH binari…