PULSATION;
MASS LOSS;
DUST;
LONG PERIOD VARIABLES;
AGB STARS;
D O I:
10.1007/BF00667917
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
We briefly discuss the current status of our radiation-hydrodynamical models of pulsation in various stellar objects and of dust-driven mass loss in LPVs, We emphasize the importance of a future combined modelling of pulsation and mass loss in AGE stars which has to be based on reliable physical and numerical methods.
机构:
LIVERPOOL JOHN MOORES UNIV,ASTROPHYS GRP,LIVERPOOL L3 3AF,MERSEYSIDE,ENGLANDLIVERPOOL JOHN MOORES UNIV,ASTROPHYS GRP,LIVERPOOL L3 3AF,MERSEYSIDE,ENGLAND
Lloyd, HM
OBrien, TJ
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机构:
LIVERPOOL JOHN MOORES UNIV,ASTROPHYS GRP,LIVERPOOL L3 3AF,MERSEYSIDE,ENGLANDLIVERPOOL JOHN MOORES UNIV,ASTROPHYS GRP,LIVERPOOL L3 3AF,MERSEYSIDE,ENGLAND
OBrien, TJ
Bode, MF
论文数: 0引用数: 0
h-index: 0
机构:
LIVERPOOL JOHN MOORES UNIV,ASTROPHYS GRP,LIVERPOOL L3 3AF,MERSEYSIDE,ENGLANDLIVERPOOL JOHN MOORES UNIV,ASTROPHYS GRP,LIVERPOOL L3 3AF,MERSEYSIDE,ENGLAND
Bode, MF
RADIO EMISSION FROM THE STARS AND THE SUN,
1996,
93
: 203
-
205