THE APPEARANCE OF HIGHLY RELATIVISTIC, SPHERICALLY SYMMETRICAL STELLAR WINDS

被引：118

作者：

ABRAMOWICZ, MA

NOVIKOV, ID

PACZYNSKI, B

机构：

[1] NORD INST TEORET FYS,COPENHAGEN,DENMARK

[2] INT CTR THEORET PHYS,I-34100 TRIESTE,ITALY

[3] PRINCETON UNIV OBSERV,PRINCETON,NJ 08544

来源：

ASTROPHYSICAL JOURNAL | 1991年 / 369卷 / 01期

关键词：

RADIATIVE TRANSFER; RELATIVITY; STARS; NEUTRON; WINDS;

D O I：

10.1086/169748

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

A nonluminous, steady state, spherically symmetric, relativistic wind, with the opacity dominated by electron scattering appears against a bright background as a dark circle with the radius r(d). A luminous wind would appear as a bright spot with a radius r(l) = r(d)/2-pi-gamma-3, where gamma is the Lorentz factor of the wind. The bright wind photosphere is convex for upsilon less-than-or-equal-to 2c/3, and appears concave for higher outflow velocities.

引用

页码：175 / 178

页数：4