Opacity in compact extragalactic radio sources and its effect on astrophysical and astrometric studies
Year: 2008
Type: article
Abstract: Context. The apparent position of the “core” in a parsec-scale radio jet (a compact, bright emitting region at the narrow end of the jet) depends on the observing frequency, owing to synchrotron self-absorption and external absorption. While providing a tool probing physical conditions in the vicinity of the core, this dependency poses problems for astrometric studies using compact radio sources.
Source: Astronomy and Astrophysics
Authors: Y. Y. Kovalev, A. P. Lobanov, A. B. Pushkarev, J. A. Zensus
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: bronze
Funders: National Science Foundation, National Aeronautics and Space Administration, Alexander von Humboldt-Stiftung, Purdue University, California Institute of Technology, National Radio Astronomy Observatory, Associated Universities, Russian Foundation for Basic Research, Jet Propulsion Laboratory, Goddard Space Flight Center
OpenAlex ID: W2105359550
