The fastest relativistic jets:: VLBA observations of blazars with apparent speeds exceeding 25c

被引:29
作者
Piner, BG
Bhattarai, D
Edwards, PG
Jones, DL
机构
[1] Whittier Coll, Dept Phys & Astron, Whittier, CA 90608 USA
[2] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[3] Inst Space & Astronaut Sci, Sagamihara, Kanagawa 2298510, Japan
关键词
BL Lacertae objects : individual (0235+164); galaxies : active; galaxies : jets; quasars : individual (0827+243,1406-076); radio continuum : galaxies;
D O I
10.1086/500006
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have measured peak apparent speeds of 25.6c +/- 7.0c, 25.6c +/- 4.4c, and 28.2c +/- 6.6c in the jets of 0235+164, 0827+243, and 1406-076, respectively, based on six epochs of high-sensitivity VLBA observations at 22 and 43 GHz during 2002 and 2003 (H-0 = 71 km s(-1) Mpc(-1), Omega(m) = 0.27, and Omega(Lambda) = 0.73). These blazars had been identified as potentially having apparent speeds exceeding 40c in an earlier VLBA survey of EGRET blazars by Jorstad and coworkers. We therefore confirm ( with high confidence in 0827+243, and lower confidence in 0235+164 and 1406-076) the presence of highly relativistic pattern speeds in these three jets, although not at the > 40c levels reported by Jorstad and coworkers. The lower limit to the bulk Lorentz factor implied by the observed apparent speeds is Gamma greater than or similar to 25-30 in these three sources, if the pattern speeds are equal to or slower than the bulk flow speed.
引用
收藏
页码:196 / 203
页数:8
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