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The Fastest Relativistic Jets: VLBA Observations of Blazars with Apparent Speeds Exceeding 25<i>c</i>

B. G. PinerDepartment of Physics and Astronomy, Whittier College, 13406 East Philadelphia Street, Whittier, CA 90608D. BhattaraiDepartment of Physics and Astronomy, Whittier College, 13406 East Philadelphia Street, Whittier, CA 90608P. G. EdwardsInstitute of Space and Astronautical Science, Yoshinodai, Sagamihara, Kanagawa 229-8510, JapanD. L. JonesJet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109
2006en
ABI

Аннотация

We have measured peak apparent speeds of 25.6 +/- 7.0c, 25.6 +/- 4.4c, and 28.2 +/- 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 Mpc), 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 et al. 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 et al. The lower limit to the bulk Lorentz factor implied by the observed apparent speeds is Gamma>25-30 in these three sources, if the pattern speeds are equal to or slower than the bulk flow speed.

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