Radiography in high mass X-ray binaries: Micro-structure of the stellar wind through variability of the column density (vol 643, A9, 2020)

被引：0

作者：

El Mellah, I. ^{[1
,3
]}

Grinberg, V. ^{[2
]}

Sundqvist, J. O. ^{[3
]}

Driessen, F. A. ^{[3
]}

Leutenegger, M. A. ^{[4
]}

机构：

[1] Katholieke Univ Leuven, Dept Math, Ctr Math Plasma Astrophys, Celestijnenlaan 200B, B-3001 Leuven, Belgium

[2] Univ Tubingen, Inst Astron & Astrophys, Sand 1, D-72076 Tubingen, Germany

[3] Katholieke Univ Leuven, Inst Astron, Celestijnenlaan 200D, B-3001 Leuven, Belgium

[4] NASA Goddard Space Flight Ctr, 8800 Greenbelt Rd, Greenbelt, MD 20771 USA

来源：

关键词：

stars: mass-loss; stars: massive; stars: winds; outflows; X-rays: binaries; radiative transfer; errata; addenda;

D O I：

10.1051/0004-6361/202038791e

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页数：1