MAPPING THE ACCRETION REGION IN AM HER SYSTEMS - ST LMI

被引：17

作者：

CROPPER, M ^{[1
]}

HORNE, K ^{[1
]}

机构：

[1] SPACE TELESCOPE SCI INST,BALTIMORE,MD 21218

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1994年 / 267卷 / 03期

关键词：

METHODS; DATA ANALYSIS; TECHNIQUES; IMAGE PROCESSING; STARS; INDIVIDUAL; ST LMI; NOVAE; CATACLYSMIC VARIABLES; X-RAYS;

D O I：

10.1093/mnras/267.3.481

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We have used the maximum entropy method to map the spatial extent of the X-ray and optical emission in the AM Her system ST LMi. The emission region is arc-shaped with a core at one extremity in the X-ray map, while the optical map is closely coincident but with some additional structure.

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页码：481 / 489

页数：9

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