VLBA23A-118

Probing the Jet Base of M87 in the Time Domain

Abstract

Recent observations of M87 with the Event Horizon Telescope have revealed a ring-like structure near the event horizon. The corresponding linear polarization images indicate that a strong, ordered, and poloidal-dominated magnetic field may exist in the vicinity of the black hole, consistent with models of AGN jet launching. However, using only the 1mm images it is difficult to understand the origin of the ring and the physical properties of the innermost accretion flows and jet base. Our recent GMVA+ALMA observations of M87 indicate that there is also a ring-like structure present at 3mm in the core of the M87 jet. Here we propose to explore a new parameter space: the time domain. We propose new observations with a global VLBI array in two epochs near in time to the planned GMVA+ALMA observations in Spring 2023. We will be able to test the jet launching models and constrain the jet acceleration mechanism by combining the global VLBI observations with the GMVA+ALMA observations, which will probe the jet base on a monthly basis for the first time. In the 2022A semester, similar observations were attempted, but our science objectives could not be achieved because ALMA's hydrogen maser failed just before the observations.

Investigators

Name Institution
Sang-Sung Lee Korea Astronomy and Space Science Institute
Do-Young Byun Korea Astronomy and Space Science Institute
Jamie Stevens Australia Telescope National Facility
Philip Edwards Australia Telescope National Facility
Chris Phillips Australia Telescope National Facility
Feng Yuan Shanghai Astronomical Observatory, CAS
Andrei Lobanov Max-Planck-Institut für Radioastronomie
zhi-qiang shen Shanghai Astronomical Observatory, CAS
Wu Jiang Shanghai Astronomical Observatory, CAS
Hung-Yi Pu Perimeter Institute for Theoretical Physics
Rusen Lu Max-Planck-Institut für Radioastronomie; Shanghai Astronomical Observatory, CAS
Tomohisa Kawashima Tokyo, University of
Jae-Young Kim Max-Planck-Institut für Radioastronomie; Kyungpook National University
Thomas Krichbaum Max-Planck-Institut für Radioastronomie
Kazuhiro Hada Istituto Nazionale di Astrofisica; National Astronomical Observatory of Japan
Fumie Tazaki National Astronomical Observatory of Japan ; Tokyo Electron Technology Solutions Ltd.
Masanori Nakamura Academia Sinica; National Institute of Technology, Hachinohe College
Keiichi Asada Academia Sinica
Jongho Park * Kyung Hee University
GBT Operator Green Bank Observatory

* indicates the PI