Merlin astrometry of 11 radio stars

被引:7
作者
Fey, AL
Boboltz, DA
Gaume, RA
Johnston, KJ
Garrington, ST
Thomasson, P
机构
[1] USN Observ, Washington, DC 20392 USA
[2] Univ Manchester, Jodrell Bank Observ, Macclesfield SK11 9DL, Cheshire, England
关键词
astrometry; radio continuum : stars; techniques : interferometric;
D O I
10.1086/498722
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report accurate positions in the International Celestial Reference Frame (ICRF) for 11 radio stars. Observations were made using the Multi-Element Radio Linked Interferometer Network at a radio frequency of 5 GHz. The positions are estimated to be accurate at the 5 mas level. Positions were obtained directly in the ICRF by phase referencing the radio stars to ICRF quasars whose positions are estimated to be accurate at the 0.25 mas level. We use our results together with results of previous observations to obtain proper-motion estimates for these stars. The average proper-motion uncertainties are 1.1 mas yr(-1) in mu(alpha cos delta) and 1.2 mas yr(-1) in mu(delta), comparable to the Hipparcos values.
引用
收藏
页码:1084 / 1089
页数:6
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