Detection of an optical/UV jet/counterjet and Multiple Spectral Components in M84
Eileen T. Meyer, Maria Petropoulou, Markos Georganopoulos, Marco, Chiaberge, Peter Breiding, William B. Sparks

TL;DR
This paper reports the discovery of an optical/UV jet and counterjet in M84, analyzes its spectral energy distribution with multi-wavelength data, and explores models to explain its complex, multi-component emission features.
Contribution
It presents the first detection of an optical/UV jet in M84 and provides a detailed spectral analysis revealing multiple co-spatial components, advancing understanding of jet emission mechanisms.
Findings
Detection of optical/UV jet and counterjet in M84
Identification of multiple spectral components in the jet
Constraints on jet orientation and proper motion
Abstract
We report an optical/UV jet and counterjet in M84, previously unreported in archival HST imaging. With archival VLA, ALMA, and Chandra imaging, we examine the first well-sampled spectral energy distribution of the inner jet of M84, where we find that multiple co-spatial spectral components are required. In particular, the ALMA data reveal that the radio spectrum of all four knots in the jet turns over at approximately 100 GHz, which requires a second component for the bright optical/UV emission. Further, the optical/UV has a soft spectrum and is inconsistent with the relatively flat X-ray spectrum, which indicates a third component at higher energies. Using archival VLA imaging, we have measured the proper motion of the innermost knots at 0.9+/-0.6 and 1.1+/-0.4 c, which when combined with the low jet-to-counterjet flux ratio yields an orientation angle for the system of 74 (+9,-18)…
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