Super-massive stars: Dense star-gas systems

被引：3

作者：

Amaro-Seoane, P ^{[1
]}

Spurzem, R ^{[1
]}

Just, A ^{[1
]}

机构：

[1] Astron Rech Inst, D-69120 Heidelberg, Germany

来源：

LIGHTHOUSES OF THE UNIVERSE: THE MOST LUMINOUS CELESTIAL OBJECTS AND THEIR USE FOR COSMOLOGY | 2002年

关键词：

D O I：

10.1007/10856495_58

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We use a gaseous model and a semi-analytical approach to study the evolution of a super-massive central gaseous object (a super-massive star, SMS from now on) in an AGN and its evolution by interactions with the surrounding stellar system. Our future work in this field is outlined, which aims at a more detailed study of energy flows in the interstellar medium, stellar evolution and the relation between QSOs and galaxy formation.

引用

页码：376 / 378

页数：3

共 12 条

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