OP VERSUS OPAL OPACITIES - CONSEQUENCES FOR B-STAR OSCILLATIONS

被引：0

作者：

PAMYATNYKH, AA

DZIEMBOWSKI, WA

MOSKALIK, P

SEATON, MJ

机构：

[1] PK SHTERNBERG ASTRON INST,MOSCOW 109017,RUSSIA

[2] UNIV LONDON UNIV COLL,DEPT PHYS & ASTRON,LONDON WC1E 6BT,ENGLAND

来源：

PULSATION, ROTATION AND MASS LOSS IN EARLY-TYPE STARS | 1994年 / 162期

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：70 / 72

页数：3

共 7 条

[1] BALONA LA, 1993, IN PRESS MNRAS
[2] DZIEMBOWSKI W, 1993, IN PRESS MNRAS
[3] THE OPACITY MECHANISM IN B-TYPE STARS .1. UNSTABLE MODES IN BETA CEPHEI STAR MODELS
DZIEMBOWSKI, WA
PAMYATNYKH, AA
[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1993, 262 (01) : 204 - 212
[4] HEYNDERICKX D, 1991, THESIS KATHOLIEKE U
[5] SPIN-ORBIT INTERACTION EFFECTS ON THE ROSSELAND MEAN OPACITY
IGLESIAS, CA
ROGERS, FJ
WILSON, BG
[J]. ASTROPHYSICAL JOURNAL, 1992, 397 (02) : 717 - 728
[6] SEATON MJ, 1993, IN PRESS MNRAS
[7] WAELKENS C, 1991, ASTRON ASTROPHYS, V246, P453