NEW OPTICAL POSITIONS OF THE GLOBULAR-CLUSTER X-RAY SOURCES NGC-6712-S X-1850-086 AND M-15-AC211 X-2127+119

被引:0
|
作者
GEFFERT, M
AURIERE, M
REQUIEME, Y
MAZURIER, JM
机构
[1] OBSERV PIC DU MIDI & TOULOUSE, CNRS, URA 1281, F-65200 BAGNERES DE BIGORRE, FRANCE
[2] OBSERV BORDEAUX, CNRS, URA 352, F-33270 FLOIRAC, FRANCE
来源
ASTRONOMY & ASTROPHYSICS | 1994年 / 282卷 / 03期
关键词
ASTROMETRY; GLOBULAR CLUSTERS; INDIVIDUAL; NGC-6712; X-RAY STARS; BINARIES; CLOSE; PULSARS; GENERAL;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Positions of the candidates for the optical counterpart of the X-ray source in the globular cluster NGC 6712 have been determined using photographic plates, image tube films, and CCD and Photon-Counting-Camera frames. The positions were determined with respect to meridian circle observations and the PPM catalogue. The small differences of the order of 0.1'' between our positions of the star called S by Nieto et al. (1990) and the radio position of Machin et al. (1990) confirm earlier suggestions that this star is indeed the optical counterpart of the X-ray source in NGC 6712. In addition, a new optical position of the X-ray source M 15:AC211/X2127+119 is given.
引用
收藏
页码:989 / 993
页数:5
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