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# Program information file
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PROGRAM_ID 2023B044
PROGRAM_TITLE Disentangling radiating particle properties and jet physics from M87 multi-wavelength variability
PROGRAM_INV1 Steven Willner
PROGRAM_INV2 Mark Gurwell
PROGRAM_INV3 Joseph Hora
PROGRAM_INV4 Daryl Haggard
PROGRAM_INV5 Sera Markoff
PROGRAM_SCICAT extra-galactic
PROGRAM_ABSTRACT_BEG
Jets from active galactic nuclei play a key role in galactic evolution. While some of the basic dynamical properties of jets are understood, the location and mechanism of particle acceleration are unknown. We propose novel observations exploiting jet variability at millimeter and near infrared wavelengths to discriminate between the three primary scenarios: 1] thermal particles dominating the inner jets, 2] nonthermal particles dominating the inner jets, and 3] thermal particles at the base, then nonthermally accelerated perhaps 100 gravitational radii from the black hole. By monitoring the inner jet emission of M87 with Gemini/GNIRS at 3.3 microns and the jet base emission with the SMA at 270 GHz, we will determine whether there is correlated variability, and if so, whether there is a time lag. The first two seasons of observations have shown correlated variability, and one or two more seasons are needed to measure the time lag. Whatever mechanism we find for M87 likely applies to many AGN jets.
PROGRAM_ABSTRACT_END