Tracing Physical Processes Affecting Spectral Formation in the Low-luminosity B[e] Stars of the FS CMa Group

被引：0

作者：

Korcakova, D. ^{[1
]}

Shore, S. N. ^{[2
]}

Miroshnichenko, A. ^{[3
,4
,5
]}

Zharikov, S. V. ^{[6
]}

Jerabkova, T. ^{[1
]}

Dvorakova, N. ^{[1
]}

Votruba, V. ^{[7
]}

Manset, N. ^{[8
]}

Slechta, M. ^{[9
]}

机构：

[1] Charles Univ Prague, Astron Inst, Prague, Czech Republic

[2] Univ Pisa, Dipartimento Fis Enrico Fermi, Pisa, Italy

[3] Univ North Carolina Greensboro, Dept Phys & Astron, Greensboro, NC USA

[4] Russian Acad Sci, Main Pulkovo Astron Observ, St Petersburg, Russia

[5] Fesenkov Astrophys Inst, Alma Ata, Kazakhstan

[6] Univ Nacl Autonoma Mexico, Inst Astron, Ensenada, Baja California, Mexico

[7] Masaryk Univ, Inst Theoret Phys & Astrophys, Brno, Czech Republic

[8] CFHT Corp, Kamuela, HI USA

[9] Acad Sci Czech Republ, Astron Inst, Ondrejov, Czech Republic

来源：

RADIATIVE SIGNATURES FROM THE COSMOS | 2019年 / 519卷

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

In order to help model the circumstellar environment of FS CMa stars, we summarize the spectral features of these objects and point to physical phenomena that affect the structure of the circumstellar region.

引用

页码：155 / 160

页数：6