The jet in the galactic center: An ideal laboratory for magnetohydrodynamics and general relativity

Heino Falcke, Sera Markoff, Geoffrey C. Bower, Charles F. Gammie, Monika Mościbrodzka, Dipankar Maitra

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

Of all possible black hole sources, the event horizon of the Galactic Center black hole, Sgr A*, subtends the largest angular scale on the sky. It is therefore a prime candidate to study and image plasma processes in strong gravity and it even allows imaging of the shadow cast by the event horizon. Recent mm-wave VLBI and radio timing observations as well as numerical GRMHD simulations now have provided several breakthroughs that put Sgr A* back into the focus. Firstly, VLBI observations have now measured the intrinsic size of Sgr A* at multiple frequencies, where the highest frequency measurements have approached the scale of the black hole shadow. Moreover, measurements of the radio variability show a clear time lag between 22 GHz and 43 GHz. The combination of size and timing measurements, allows one to actually measure the flow speed and direction of magnetized plasma at some tens of Schwarzschild radii. This data strongly support a moderately relativistic outflow, consistent with an accelerating jet model. This is compared to recent GRMHD simulation that show the presence of a moderately relativistic outflow coupled to an accretion flow Sgr A*. Further VLBI and timing observations coupled to simulations have the potential to map out the velocity profile from 5-40 Schwarzschild radii and to provide a first glimpse at the appearance of a jet-disk system near the event horizon. Future submm-VLBI experiments would even be able to directly image those processes in strong gravity and directly confirm the presence of an event horizon.

Original languageEnglish (US)
Title of host publicationJets at all Scales
EditorsGustavo Romero, Rashid Sunyaev, Rashid Sunyaev, Tomaso Belloni
Pages68-76
Number of pages9
EditionS275
DOIs
StatePublished - Sep 1 2010

Publication series

NameProceedings of the International Astronomical Union
NumberS275
Volume6
ISSN (Print)1743-9213
ISSN (Electronic)1743-9221

Keywords

  • Accretion
  • Black hole physics
  • Galaxies: jets
  • Galaxy: center
  • Galaxy: nucleus
  • Gravitation
  • Instrumentation: high angular resolution
  • Instrumentation: interferometers
  • MHD
  • Quasars: general
  • Relativity

ASJC Scopus subject areas

  • Medicine (miscellaneous)
  • Astronomy and Astrophysics
  • Nutrition and Dietetics
  • Public Health, Environmental and Occupational Health
  • Space and Planetary Science

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    Falcke, H., Markoff, S., Bower, G. C., Gammie, C. F., Mościbrodzka, M., & Maitra, D. (2010). The jet in the galactic center: An ideal laboratory for magnetohydrodynamics and general relativity. In G. Romero, R. Sunyaev, R. Sunyaev, & T. Belloni (Eds.), Jets at all Scales (S275 ed., pp. 68-76). (Proceedings of the International Astronomical Union; Vol. 6, No. S275). https://doi.org/10.1017/S1743921310015656