AN EPHEMERIS FOR THE INTERMEDIATE POLAR RE-0751+14

被引：19

作者：

HELLIER, C ^{[1
]}

RAMSEYER, TF ^{[1
]}

JABLONSKI, FJ ^{[1
]}

机构：

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

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1994年 / 271卷 / 02期

关键词：

ACCRETION; ACCRETION DISKS; BINARIES; CLOSE; STARS; INDIVIDUAL; RE; 0751; 14; MAGNETIC FIELDS; NOVAE; CATACLYSMIC VARIABLES;

D O I：

10.1093/mnras/271.1.L25

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

RE 0751 + 14 shows an 833-s spin pulsation which is quasi-sinusoidal in the blue, but double-peaked in the red. We present the first ephemeris for this pulsation. A weaker 872-s pulsation is also double-peaked, and is probably caused by reprocessing of the double-peaked X-ray pulse. The optical modulation at the implied orbital period is weaker than in any other intermediate polar, which suggests that RE 0751 + 14 is at a low inclination.

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页码：L25 / L29

页数：5

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