THE HIGH-OVERTONE P-MODE SPECTRUM OF THE RAPIDLY OSCILLATING AP STAR HR-1217 (HD 24712) - RESULTS OF A FREQUENCY-ANALYSIS OF 324 HR OF MULTI-SITE PHOTOMETRIC-OBSERVATIONS OBTAINED DURING A 46-D TIME-SPAN IN 1986

被引：74

作者：

KURTZ, DW

MATTHEWS, JM

MARTINEZ, P

SEEMAN, J

CROPPER, M

CLEMENS, JC

KREIDL, TJ

STERKEN, C

SCHNEIDER, H

WEISS, WW

KAWALER, SD

KEPLER, SO

机构：

[1] UNIV WESTERN ONTARIO,DEPT ASTRON,LONDON N6A 3K7,ONTARIO,CANADA

[2] ANGLO AUSTRALIAN OBSERV,EPPING,NSW 2121,AUSTRALIA

[3] UNIV TEXAS,DEPT ASTRON,AUSTIN,TX 78712

[4] LOWELL OBSERV,FLAGSTAFF,AZ 86001

[5] VRIJE UNIV BRUSSELS,INST ASTROPHYS,B-1050 BRUSSELS,BELGIUM

[6] UNIV STERNWARTE GOTTINGEN,D-3400 GOTTINGEN,FED REP GER

[7] INST ASTRON,A-1180 VIENNA,AUSTRIA

[8] YALE UNIV,CTR SOLAR & SPACE RES,NEW HAVEN,CT 06511

[9] UNIV FED RIO GRANDE DO SUL,INST FIS,BR-90049 PORTO ALEGRE,RS,BRAZIL

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1989年 / 240卷 / 04期

关键词：

D O I：

10.1093/mnras/240.4.881

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：881 / 915

页数：35

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