Mou, Jian
Chen, Hai-Liang
Jiang, Dengkai https://orcid.org/0000-0003-4265-7783
Ge, Hongwei https://orcid.org/0000-0002-6398-0195
Zhang, Lifu
Zheng, Rizhong
Chen, Xuefei https://orcid.org/0000-0001-5284-8001
Han, Zhanwen https://orcid.org/0000-0001-9204-7778
Funding for this research was provided by:
MOST ∣ National Natural Science Foundation of China (12288102)
MOST ∣ National Natural Science Foundation of China (12090040/12090043)
MOST ∣ National Natural Science Foundation of China (12333008)
MOST ∣ National Natural Science Foundation of China (12422305)
MOST ∣ National Natural Science Foundation of China (12473033)
MOST ∣ National Natural Science Foundation of China (12525304)
MOST ∣ National Natural Science Foundation of China (12125303)
MOST ∣ National Key Research and Development Program of China (2021YFA1600400/401)
MOST ∣ National Key Research and Development Program of China (2021YFA1600403)
Strategic Priority Research Program of the Chinese Academy of Sciences (XDB1160201)
CAS "Light of West China"
Young Talent Project of Yunnan Revitalization Talent Support Program
Yunnan Fundamental Research Project (202401BC070007)
Yunnan Revitalization Talent Support Program-Science & Technology Champion Project (202305AB35003)
International Center of Supernovae (202201BC070003)
Yunnan Key Laboratory (202302AN360001)
Article Title: The Relation between Helium White Dwarf Mass and Orbital Period under Two Types of Opacity
Journal Title: The Astrophysical Journal
Article Type: paper
Copyright Information: © 2025. The Author(s). Published by the American Astronomical Society.
Publication dates
Date Received: 2025-10-24
Date Accepted: 2025-11-21
Online publication date: 2025-12-29