pith. sign in

arxiv: 1804.03776 · v1 · pith:4RKR6HCUnew · submitted 2018-04-11 · 🌌 astro-ph.GA · astro-ph.HE

A Recollimation Shock in a Stationary Jet Feature with Limb-brightening in the Gamma-ray Emitting Narrow-line Seyfert 1 Galaxy 1H 0323+342

classification 🌌 astro-ph.GA astro-ph.HE
keywords convergencefeaturequasi-stationarysitegalaxygamma-raygamma-ray-emittinglimb-brightening
0
0 comments X p. Extension
pith:4RKR6HCU Add to your LaTeX paper What is a Pith Number?
\usepackage{pith}
\pithnumber{4RKR6HCU}

Prints a linked pith:4RKR6HCU badge after your title and writes the identifier into PDF metadata. Compiles on arXiv with no extra files. Learn more

read the original abstract

We report the discovery of a local convergence of a jet cross section in the quasi-stationary jet feature in the gamma-ray-emitting narrow-line Seyfert 1 galaxy (NLS1) 1H 0323+342. The convergence site is located at approximately 7 mas (corresponding to the order of 100 pc in deprojection) from the central engine. We also found limb-brightened jet structures at both the upstream and downstream of the convergence site. We propose that the quasi-stationary feature showing the jet convergence and limb-brightening occurs as a consequence of recollimation shock in the relativistic jets. The quasi-stationary feature is one of the possible gamma-ray-emitting sites in this NLS1, in analogy with the HST-1 complex in the M87 jet. Monitoring observations have revealed that superluminal components passed through the convergence site and the peak intensity of the quasi-stationary feature, which showed apparent coincidences with the timing of observed gamma-ray activities.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.