X-RAY-EMISSION FROM AN AP-STAR (PHI-HERCULIS) AND A LATE B-STAR (PI-CETI)

被引：18

作者：

CASH, W

SNOW, TP

CHARLES, P

机构：

[1] UNIV COLORADO,DEPT ASTROGEOPHYS,BOULDER,CO 80309

[2] UNIV CALIF BERKELEY,SPACE SCI LAB,BERKELEY,CA 94720

来源：

ASTROPHYSICAL JOURNAL | 1979年 / 232卷 / 02期

关键词：

D O I：

10.1086/183046

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：L111 / L115

页数：5

共 33 条

[1]

Babcock H. W., 1958, ASTROPHYS J, V3, P141, DOI DOI 10.1086/190035

[2]

Bevington PR., 2003, DATA REDUCTION ERROR

[3]

CAMERON RC, 1967, MAGNETIC RELATED STA

[4] EXTREME ULTRAVIOLET OBSERVATION OF SIRIUS - EVIDENCE AGAINST A PHOTOSPHERIC ORIGIN OF 0.25 KEV FLUX [J].

CASH, W ;

BOWYER, S ;

LAMPTON, M .

ASTROPHYSICAL JOURNAL, 1978, 221 (02) :L87-L89

[5]

CASH W, 1976, ASTRON ASTROPHYS, V52, P307

[6] SOFT-X-RAY SPECTRUM OF CAPELLA - DISCOVERY OF INTENSE LINE EMISSION [J].

CASH, W ;

BOWYER, S ;

CHARLES, PA ;

LAMPTON, M ;

GARMIRE, G ;

RIEGLER, G .

ASTROPHYSICAL JOURNAL, 1978, 223 (01) :L21-L23

[7]

CASH WD, UNPUBLISHED

[8]

CATALANO FA, 1976, P IAU C, P63

[9] METALLIC-LINE STARS [J].

CONTI, PS .

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 1970, 82 (488) :781-&

[10]

de Loore C., 1970, Astrophysics and Space Science, V6, P60, DOI 10.1007/BF00653620

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