Search for Cataclysmic Variables Based on the 400d X-ray Sky Survey

被引:3
作者
Tkachenko, A. Yu. [1 ]
Revnivtsev, M. G. [1 ]
Burenin, R. A. [1 ]
Meshcheryakov, A. V. [1 ]
Vorob'ev, V. S. [1 ]
Pavlinsky, M. N. [1 ]
机构
[1] Russian Acad Sci, Space Res Inst, Moscow 117997, Russia
来源
ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS | 2015年 / 41卷 / 05期
基金
俄罗斯基础研究基金会;
关键词
X-ray sources; cataclysmic variables; optical observations; LUMINOSITY FUNCTION; SPACE DENSITY; DWARF NOVAE; POPULATION; EMISSION; CONSTRAINTS; SAMPLE; CALIBRATION; ORIGIN; PERIOD;
D O I
10.1134/S1063773715050084
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the first results of our search for cataclysmic variables among the point X-ray sources detected in a part of the sky survey with an area of 400 sq. deg. performed on the basis of data from the ROSAT telescope (400d), for which photometric data from the Sloan Digital Sky Survey are also available. The necessary optical observations of the candidates for cataclysmic variables have been carried out with the 1.5-m Russian-Turkish telescope (RTT-150). We show that one of the four investigated objects (400D J0019126+220733) is a cataclysmic variable, two objects are quasars at redshifts z similar to 2, and the nature of one object remains unclarified; however, we can exclude it from the list of possible candidates for cataclysmic variables: its spectrum contains no characteristic emission features.
引用
收藏
页码:174 / 178
页数:5
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