FATE OF MERGING DOUBLE WHITE-DWARFS .2. NUMERICAL-METHOD

被引：23

作者：

HACHISU, I

ERIGUCHI, Y

NOMOTO, K

机构：

[1] KYOTO UNIV,DEPT AERONAUT ENGN,KYOTO 606,JAPAN

[2] UNIV TOKYO,COLL ARTS & SCI,DEPT EARTH SCI & ASTRON,MEGURO KU,TOKYO 153,JAPAN

[3] BROOKHAVEN NATL LAB,DEPT PHYS,UPTON,NY 11973

来源：

ASTROPHYSICAL JOURNAL | 1986年 / 311卷 / 01期

关键词：

D O I：

10.1086/164766

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：214 / 225

页数：12

共 11 条

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[6] 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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IBEN, I .

ASTROPHYSICAL JOURNAL, 1985, 297 (02) :531-537

[7] RAPIDLY ROTATING STARS .I. SELF-CONSISTENT-FIELD METHOD [J].

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[8]

SAIO H, 1985, ASTRON ASTROPHYS, V150, pL21

[9]

Tutukov A. V., 1979, Acta Astronomica, V29, P665

[10] DOUBLE WHITE-DWARFS AS PROGENITORS OF R CORONAE BOREALIS STARS AND TYPE-I SUPERNOVAE [J].

WEBBINK, RF .

ASTROPHYSICAL JOURNAL, 1984, 277 (01) :355-360

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