Chandra localization of XTE J1906+090 and discovery of its optical and infrared counterparts

被引:8
作者
Gögüs, E
Patel, SK
Wilson, CA
Woods, PM
Finger, MH
Kouveliotou, C
机构
[1] Sabanci Univ, Fac Engn & Nucl Sci, TR-34956 Istanbul, Turkey
[2] Univ Space Res Assoc, Seabrook, MD 20706 USA
[3] Natl Space Sci & Technol, Space Sci Branch, Huntsville, AL 35805 USA
[4] NASA, George C Marshall Space Flight Ctr, Huntsville, AL 35812 USA
关键词
infrared : stars; pulsars : individual ( XTE J1906+090); X-rays : binaries;
D O I
10.1086/444373
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the Chandra identification and localization of the transient X-ray source XTE J1906+090 and the discovery of its optical and infrared counterparts. Our analysis of archival Chandra ACIS-I observations of the field found the source approximately 80 away from the position determined earlier with the RXTE PCA. We have confirmed the source identification with timing analysis of the X-ray data, which detected the source spin period of 89.6 s. The best Chandra position for the source is R.A. = 19(h)04(m)47(s).491, decl = +09 degrees 02'41."40. Subsequently, we performed optical observations of the field around the new location and discovered a coincident optical source with R-band magnitude of 18.7. A search in the Two Micron All Sky Survey catalog revealed an infrared point source with J = 15.2, H = 14.2, and K = 13.5, whose location is also coincident with our Chandra and optical positions. Our results add fresh evidence for a Be/X-ray transient nature for XTE J1906+090.
引用
收藏
页码:1069 / 1074
页数:6
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