STEADY-STATE MODELS OF WHITE-DWARFS ACCRETING HELIUM OR CARBON OXYGEN RICH MATTER

被引：23

作者：

KAWAI, Y ^{[1
]}

SAIO, H ^{[1
]}

NOMOTO, K ^{[1
]}

机构：

[1] UNIV TOKYO,COLL ARTS & SCI,DEPT EARTH SCI & ASTRON,TOKYO 153,JAPAN

来源：

ASTROPHYSICAL JOURNAL | 1988年 / 328卷 / 01期

关键词：

D O I：

10.1086/166282

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：207 / 212

页数：6

共 20 条

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[10] CARBON IGNITION IN A RAPIDLY ACCRETING DEGENERATE DWARF - A CLUE TO THE NATURE OF THE MERGING PROCESS IN CLOSE BINARIES [J].

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