期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 507, 期 3, 页码 4603-4617出版社
OXFORD UNIV PRESS
DOI: 10.1093/mnras/stab2369
关键词
stars: chemically peculiar; stars: kinematics and dynamics; subdwarfs; supernovae: general
资金
- Natural Science Foundation of China [11973080, 11733008, U173111]
- China Manned Space Project [CMSCSST-2021-B07]
- Yunnan Ten Thousand Talents Plan - Young & Elite Talents Project
- CAS 'Light of West China' Program
This paper investigates the evolution of surviving companions from the white dwarf + main-sequence channel into hot subdwarfs, and presents the Galactic birth rate of hot subdwarfs from this channel. The study suggests that these hot subdwarfs may help explain observational features of intermediate helium-rich hot subdwarfs, particularly those from the spin-up/spin-down model.
Some surviving companions of Type Ia supernovae (SNe Ia) from the white dwarf + main-sequence (WD+MS) channel may evolve to hot subdwarfs. In this paper, we perform stellar evolution calculations for the surviving companions of close WD+MS systems in the spin-up/spin-down model and the canonical non-rotating model. This enables us to map out the initial parameter spaces in the orbital period-secondary-mass plane in which the surviving companions can evolve to hot subdwarfs. Based on these results, we carry out a series of binary population synthesis calculations to obtain the Galactic birth rate of hot subdwarfs from the WD+MS channel, which is 2.3-6x10(-4)yr(-1) for the spin-up/spin-down model and 0.7-3x10(-4)yr(-1) for the canonical non-rotating model. We also show the distributions of some integral properties of the hot subdwarfs, for example the mass and space velocity, for different models. In addition, by comparing our results with observations of intermediate helium-rich (iHe-rich) hot subdwarfs, we find that the hot subdwarfs from the WD+MS channel may explain some observational features of the iHe-rich hot subdwarfs, especially those from the spin-up/spin-down model. Although we expect that the SN Ia channel will contribute only a small fraction of the iHe-rich hot subdwarf population, some of these may help to explain cases with unusual kinematics.
作者
我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。
推荐
暂无数据