THE X-RAY-PROPERTIES OF AM CANUM-VENATICORUM

被引：0
作者：
ULLA, A [1 ]
机构：
[1] INTA, ASTROFIS ESPACIAL & FIS FUNDAMENTAL LAB, E-28080 MADRID, SPAIN
来源：
ASTRONOMY & ASTROPHYSICS | 1995年 / 301卷 / 02期
关键词：
STARS; AM CVN; CATACLYSMIC VARIABLES; X-RAYS;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Archival X-ray observations of AM CVn are analysed and the obtained results are presented. Its once reported Ariel V hard X-ray emission detection is discarded in the light of the new data. In particular, soft X-rays are unambiguously detected for the first time by the ROSAT Satellite. X-ray luminosities of the order of only 10(29) erg s(-1) are derived, posing some constraints on the possible nature of AM CVn. The implications following our analysis are discussed in the cataclysmic variables' context.
引用
收藏
页码：469 / 477
页数：9
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