Confronting consistent dust shell models with observations of long-period variable stars

被引：0

作者：

Winters, JM ^{[1
]}

机构：

[1] Max Planck Inst Radioastron, D-53121 Bonn, Germany

来源：

MASS-LOSING PULSATING STARS AND THEIR CIRCUMSTELLAR MATTER: OBSERVATIONS AND THEORY | 2003年 / 283卷

关键词：

hydrodynamics; mass-loss; outflows; dust;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The ingredients necessary for a consistent description of dust forming atmospheres around pulsating stars are addressed and the results of corresponding hydrodynamical model calculations are compared with respective observations.

引用

页码：151 / 158

页数：8

共 32 条

[1] Electronic structure investigation of the Al4O4 molecule [J].

Chang, C ;

Patzer, ABC ;

Sedlmayr, E ;

Steinke, T ;

Sülzle, D .

CHEMICAL PHYSICS LETTERS, 2000, 324 (1-3) :108-114

[2]

DOMINIK C, 1993, ASTRON ASTROPHYS, V277, P578

[3]

DOMINIK C, 1989, ASTRON ASTROPHYS, V223, P227

[4]

FLEISCHER AJ, 1995, ASTRON ASTROPHYS, V297, P543

[5]

Gail HP, 1999, ASTRON ASTROPHYS, V347, P594

[6]

GAIL HP, 1986, ASTRON ASTROPHYS, V166, P225

[7]

GAIL HP, 1988, ASTRON ASTROPHYS, V206, P153

[8]

GAUGER A, 1990, ASTRON ASTROPHYS, V235, P345

[9]

Haniff CA, 1998, ASTRON ASTROPHYS, V334, pL5

[10]

HOFNER S, 1995, ASTRON ASTROPHYS, V297, P815

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