10–12 Mar 2025
Osaka University Nakanoshima Center
Asia/Tokyo timezone

ALMA Continuum Observations of NGC 1068 and GRS 1734-292

10 Mar 2025, 15:05
40m
セミナー室6E+F (Osaka University Nakanoshima Center)

セミナー室6E+F

Osaka University Nakanoshima Center

〒530-0005 大阪市北区中之島4-3-53

Speaker

Tomonari Michiyama (Shunan University)

Description

"I summarize three ALMA studies investigating jet and coronal activities in Seyfert galaxies.

NGC 1068 Jet: High-resolution ALMA observations reveal parsec-scale blobs in the jet of NGC 1068, with a magnetic field of ≈240 μG. These findings suggest cosmic-ray amplification and significant galactic impact even from modest-power jets.

NGC 1068 Core Spectrum: Broad-band data from 5–700 GHz, including new ALMA results, indicate a combination of emission from the jet base, dusty torus, and compact corona. Updated models suggest a strong magnetic field near the black hole, but higher-resolution data are needed to confirm.

GRS 1734-292 Variability: ALMA detected millimeter excess and time variability in the central ≲100 pc of this radio-quiet galaxy. The findings suggest synchrotron emission from a compact corona or disk winds, with future high-resolution observations required to differentiate these scenarios."

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