THE EFFECT OF A BINARY COMPANION ON A NOVA OUTBURST

被引：60

作者：

MACDONALD, J ^{[1
]}

机构：

[1] INST ASTRON,CAMBRIDGE CB3 0HA,ENGLAND

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1980年 / 191卷 / 03期

关键词：

D O I：

10.1093/mnras/191.4.933

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We compare two calculations of thermonuclear runaways in solar composition material (Z = 0.02) accreted by a 1M☉ white dwarf. We include the interaction of the expanding envelope with a red dwarf companion in only one of the evolutionary sequences. A slow nova results when this binary interaction is included but when it is omitted the outbursts more nearly resemble the very slow novae, like RR Tel and RT Ser. © Royal Astronomical Society.

引用

页码：933 / 949

页数：17

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