Unveiling Ionized Jet Morphologies: Sub-arcsecond VLA Observations of Compact Radio Sources
Tatiana M. Rodriguez (1), Peter Hofner (2, 3), Emmanuel Momjian (4), Esteban D. Araya (5, 2), Ananay Sethi (2), Viviana Rosero (6) ((1) University of Cologne, (2) New Mexico Institute of Mining, Technology, (3) Adjunct Astronomer at the National Radio Astronomy Observatory

TL;DR
This study uses high-resolution VLA observations to analyze the morphologies and dynamics of ionized jets in compact radio sources, revealing diverse structures, proper motions, and variability that support shock ionization and jet classification.
Contribution
It provides detailed morphological, kinematic, and variability data on ionized jets in compact sources, enhancing understanding of their structures and ionization mechanisms.
Findings
Multiple jet morphologies observed, including string-like and compact sources.
Proper motions with an average velocity of 120 km/s detected in 10 sources.
Evidence supporting shock ionization as the main ionization mechanism.
Abstract
We present sub-arcsecond () resolution VLA 1.3 cm continuum and 22.2 GHz HO maser observations toward 15 compact radio continuum sources with rising spectral index and 8 string-like radio continuum structures in the Rosero et al. (2016, 2019) survey. Three different morphologies are observed: elongated or double-peak string-like structure (6 out of 23 cases), a collection of distinct continuum peaks (4 out of 23 cases), and single compact sources (13 out of 23 cases). The majority of HO maser spots detected are within a sky-projected distance of au from the radio continuum peaks and tend to be well aligned and distributed in an elongated structure when more than three spots are observed. We generally recover less emission than Rosero et al. (2016, 2019), which together with the fact that more than half of the jet candidates in our survey…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Astrophysical Phenomena and Observations · Galaxies: Formation, Evolution, Phenomena
