A magnetic dynamo origin for the submillimeter excess in sagittarius A

Fulvio Melia, Siming Liu, Robert Coker

Research output: Contribution to journalArticle

34 Citations (Scopus)

Abstract

The submillimeter bump observed in the spectrum of Sgr A * appears to indicate the existence of a compact emitting component within several Schwarzschild radii, rs, of the nucleus at the Galactic center. This is interesting in view of the predicted circularized flow within ∼5-10rs, based on detailed multidimensional hydrodynamic simulations of Bondi-Hoyle accretion onto this unusual object. In this paper, we examine the physics of magnetic field generation by a Keplerian dynamo subject to the conditions pertaining to Sgr A *, and show that the submillimeter bump can be produced by thermal synchrotron emission in this inner region. This spectral feature may therefore be taken as indirect evidence for the existence of this circularization. In addition, the self-Comptonization of the submillimeter bump appears to produce an X-ray flux exceeding that due to bremsstrahlung from this region, which may account for the X-ray counterpart to Sgr A * discovered recently by Chandra. However, the required accretion rate in the Keplerian flow is orders of magnitude smaller than that predicted by the Bondi-Hoyle simulations. We speculate that rapid evaporation, in the form of a wind, may ensue from the heating associated with turbulent mixing of gas elements with large eccentricity as they settle down into a more or less circular (i.e., low-eccentricity) trajectory. The spectrum of Sgr A * longward of ∼1-2 mm may be generated outside of the Keplerian flow, where the gas is making a transition from a quasi-spherical infall to a circularized pattern.

Original languageEnglish (US)
Pages (from-to)146-157
Number of pages12
JournalAstrophysical Journal
Volume553
Issue number1 PART 1
DOIs
StatePublished - May 20 2001

Fingerprint

eccentricity
accretion
turbulent mixing
gases
gas
bremsstrahlung
simulation
synchrotrons
x rays
physics
evaporation
hydrodynamics
trajectory
trajectories
magnetic field
heating
nuclei
radii
magnetic fields
rate

Keywords

  • Accretion, accretion disks
  • Black hole physics
  • Galaxy: Center
  • Hydrodynamics
  • Magnetic fields
  • MHD

ASJC Scopus subject areas

  • Space and Planetary Science

Cite this

A magnetic dynamo origin for the submillimeter excess in sagittarius A. / Melia, Fulvio; Liu, Siming; Coker, Robert.

In: Astrophysical Journal, Vol. 553, No. 1 PART 1, 20.05.2001, p. 146-157.

Research output: Contribution to journalArticle

Melia, Fulvio ; Liu, Siming ; Coker, Robert. / A magnetic dynamo origin for the submillimeter excess in sagittarius A. In: Astrophysical Journal. 2001 ; Vol. 553, No. 1 PART 1. pp. 146-157.
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