盘吸积时低磁场中子星边界层的近似解析模型

IF 0.7 4区物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS

Astrophysics Pub Date : 2025-08-19 DOI:10.1007/s10511-025-09869-y

G. S. Bisnovatyi-Kogan

引用次数: 0

摘要

我们建立了中子星周围吸积盘边界层的近似解析一维模型，该中子星的低磁场不影响吸积过程。我们考虑了一个高光度模型，辐射压力在盘的内部占主导地位。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

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Approximate Analytic Model of the Boundary Layer Arround a Low Magnetic Field Neutron Star at the Disk Accretion

We have constructed an approximate analytic one-dimensional model of the accretion disk boundary layer surrounding a neutron star whose low magnetic field does not affect the process of accretion. We consider a high luminosity model with radiation pressure dominant in the interior part of the disk.

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来源期刊

Astrophysics 地学天文-天文与天体物理

CiteScore

0.90

自引率

20.00%

发文量

审稿时长

6-12 weeks

期刊介绍： Astrophysics (Ap) is a peer-reviewed scientific journal which publishes research in theoretical and observational astrophysics. Founded by V.A.Ambartsumian in 1965 Astrophysics is one of the international astronomy journals. The journal covers space astrophysics, stellar and galactic evolution, solar physics, stellar and planetary atmospheres, interstellar matter. Additional subjects include chemical composition and internal structure of stars, quasars and pulsars, developments in modern cosmology and radiative transfer.