The Radio Structure of High-Energy–Peaked BL Lacertae Objects

  • Rector T
  • Gabuzda D
  • Stocke J
57Citations
Citations of this article
7Readers
Mendeley users who have this article in their library.

Abstract

We present VLA and first-epoch VLBA observations that are part of a program to study the parsec-scale radio structure of a sample of fifteen high-energy-peaked BL Lacs (HBLs). The sample was chosen to span the range of logarithmic X-ray to radio flux ratios observed in HBLs. As this is only the first epoch of observations, proper motions of jet components are not yet available; thus we consider only the structure and alignment of the parsec- and kiloparsec-scale jets. Like most low-energy-peaked BL Lacs (LBLs), our HBL sample shows parsec-scale, core-jet morphologies and compact, complex kiloparsec-scale morphologies. Some objects also show evidence for bending of the jet 10-20pc from the core, suggesting interaction of the jet with the surrounding medium. Whereas LBLs show a wide distribution of parsec- to kpc-scale jet misalignment angles, there is weak evidence that the jets in HBLs are more well-aligned, suggesting that HBL jets are either intrinsically straighter or are seen further off-axis than LBL jets.

Cite

CITATION STYLE

APA

Rector, T. A., Gabuzda, D. C., & Stocke, J. T. (2003). The Radio Structure of High-Energy–Peaked BL Lacertae Objects. The Astronomical Journal, 125(3), 1060–1072. https://doi.org/10.1086/367802

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free