2009A&A...496...77F


C.D.S. - SIMBAD4 rel 1.7 - 2021.02.26CET09:34:32

2009A&A...496...77F - Astronomy and Astrophysics, volume 496, 77-83 (2009/3-2)

Jet-lag in Sagittarius A*: what size and timing measurements tell us about the central black hole in the Milky way.

FALCKE H., MARKOFF S. and BOWER G.C.

Abstract (from CDS):

The black hole at the Galactic Center, Sgr A*, is the prototype of a galactic nucleus at a very low level of activity. Its radio through submm-wave emission is known to come from a region close to the event horizon, however, the source of the emission is still under debate. A successful theory explaining the emission is based on a relativistic jet model scaled down from powerful quasars. We want to test the predictive power of this established jet model against newly available measurements of wavelength-dependent time lags and the size-wavelength structure in Sgr A*. Using all available closure amplitude VLBI data from different groups, we again derived the intrinsic wavelength-dependent size of Sgr A*. This allowed us to calculate the expected frequency-dependent time lags of radio flares, assuming a range of in- and outflow velocities. Moreover, we calculated the time lags expected in the previously published pressure-driven jet model. The predicted lags are then compared to radio monitoring observations at 22, 43, and 350GHz. The combination of time lags and size measurements imply a mildly relativistic outflow with bulk outflow speeds of γβ≃0.5-2. The newly measured time lags are reproduced well by the jet model without any major fine tuning. The results further strengthen the case for the cm-to-mm wave radio emission in Sgr A* as coming from a mildly relativistic jet-like outflow. The combination of radio time lag and VLBI closure amplitude measurements is a powerful new tool for assessing the flow speed and direction in Sgr A*. Future VLBI and time lag measurements over a range of wavelengths will reveal more information about Sgr A*, such as the existence of a jet nozzle, and measure the detailed velocity structure of a relativistic jet near its launching point for the first time.

Abstract Copyright:

Journal keyword(s): black hole physics - galaxies: active - galaxies: jets - galaxies: nuclei - Galaxy: center - radio continuum: general

Simbad objects: 3

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Number of rows : 3

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2021
#notes
1 M 81 Sy2 09 55 33.17306143 +69 03 55.0609270   7.89 6.94     ~ 4042 5
2 NAME Sgr A* X 17 45 40.03599 -29 00 28.1699           ~ 3597 3
3 NAME Gal Center reg 17 45 40.04 -29 00 28.1           ~ 11994 0

    Equat.    Gal    SGal    Ecl

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