RXJ 0929.1-2404 - AN ECLIPSING MAGNETIC CATACLYSMIC VARIABLE

被引：8

作者：

SEKIGUCHI, K

NAKADA, Y

BASSETT, B

机构：

[1] UNIV TOKYO,INST ASTRON,KISO OBSERV,MITAKE,NAGANO 39701,JAPAN

[2] UNIV CAPE TOWN,DEPT APPL MATH,RONDEBOSCH 7700,SOUTH AFRICA

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1994年 / 266卷 / 03期

关键词：

BINARIES; ECLIPSING; STARS; INDIVIDUAL; RXJ; 0929.1-2404; NOVAE; CATACLYSMIC VARIABLES; X-RAYS;

D O I：

10.1093/mnras/266.1.L51

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Optical photometry of the X-ray source RXJ 0929.1 - 2404 reveals deep recurrent eclipses. Observations presently available are consistent with RXJ 0929.1 - 2404 being a polar with an orbital period of 3.39 h, placing it somewhat above the cataclysmic variable 'period gap'. In fact, this establishes RXT 0929.1 - 2404 as the only eclipsing polar with a period above the 'period gap'.

引用

页码：L51 / L53

页数：3

共 7 条

[1]

[Anonymous], 1989, S AFRICAN ASTRON OBS

[2] DISCOVERY OF AN EUV-BRIGHT POLAR IN THE PERIOD GAP FROM THE ROSAT WIDE-FIELD CAMERA SKY SURVEY [J].