BINARY STAR MODEL FOR SS433

被引：9

作者：

DEYOUNG, DS ^{[1
]}

BURBIDGE, G ^{[1
]}

机构：

[1] KITT PEAK NATL OBSERV,TUCSON,AZ 85726

来源：

NATURE | 1979年 / 281卷 / 5728期

关键词：

D O I：

10.1038/281183a0

中图分类号：

O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];

学科分类号：

07 ; 0710 ; 09 ;

摘要：

The novel features recently observed for the strong emission line object SS433 can be explained by a model in which SS433 is a binary of a massive early-type star and a magnetic white dwarf. © 1979 Nature Publishing Group.

引用

页码：183 / 185

页数：3

共 14 条

[1] KINEMATIC MODEL FOR SS433 [J].

ABELL, GO ;

MARGON, B .

NATURE, 1979, 279 (5715) :701-703

[2]

ANGEL JRP, 1978, REV ASTR ASTROPHYS, V16, P487

[3] X-RAY-EMISSION FROM ACCRETION ON TO WHITE-DWARFS [J].

FABIAN, AC ;

PRINGLE, JE ;

REES, MJ .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1976, 175 (01) :43-60

[4] SS-433 - DOUBLE JET IN ACTION [J].

FABIAN, AC ;

REES, MJ .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1979, 187 (01) :P13-P16

[5]

GOLDSTEIN H, 1950, CLASSICAL MECHANICS, P182

[6] MOVING EMISSION FEATURES IN SS433 REQUIRE A DYNAMICAL INTERPRETATION [J].

LIEBERT, J ;

ANGEL, JRP ;

HEGE, EK ;

MARTIN, PG ;

BLAIR, WP .

NATURE, 1979, 279 (5712) :384-387

[7]

LIEBERT J, ASTROPHYS J

[8] BIZARRE SPECTRUM OF SS-433 [J].

MARGON, B ;

FORD, HC ;

KATZ, JI ;

KWITTER, KB ;

ULRICH, RK ;

STONE, RPS ;

KLEMOLA, A .

ASTROPHYSICAL JOURNAL, 1979, 230 (01) :L41-L45

[9]

MARGON B, 1979, IAU3345 CIRC

[10]

MCGRAW J, 1979, IAU3363 CIRC

← 1 2 →