Polarimetric imaging of the massive black hole at the galactic center

Benjamin C. Bromley, Fulvio Melia, Siming Liu

Research output: Contribution to journalArticle

67 Citations (Scopus)

Abstract

The radio source Sagittarius A* in the Galactic center emits a polarized spectrum at millimeter and submillimeter wavelengths that is strongly suggestive of relativistic disk accretion onto a massive black hole. We use the well-constrained mass of Sgr A* and a magnetohydrodynamic model of the accretion flow to match both the total flux and polarization from this object. Our results demonstrate explicitly that the shift in the position angle of the polarization vector, seen at wavelengths near the peak of the millimeter to submillimeter emission from this source, is a signal of relativistic accretion flow in a strong gravitational field. We provide maps of the polarized emission to illustrate how the images of polarized intensity from the vicinity of the black hole would appear in upcoming observations with very long baseline radio interferometers (VLBIs). Our results suggest that near-term VLBI observations will be able to directly image the polarized Keplerian portion of the flow near the horizon of the black hole.

Original languageEnglish (US)
JournalAstrophysical Journal
Volume555
Issue number2 PART 2
DOIs
StatePublished - Jul 10 2001

Fingerprint

radio interferometers
accretion
radio
interferometer
polarization
wavelength
magnetohydrodynamics
wavelengths
accretion disks
gravitational fields
horizon
shift

Keywords

  • Accretion, accretion disks
  • Black hole physics
  • Galaxy: center
  • Hydrodynamics
  • Magnetic fields
  • Radiation mechanisms: nonthermal

ASJC Scopus subject areas

  • Space and Planetary Science

Cite this

Polarimetric imaging of the massive black hole at the galactic center. / Bromley, Benjamin C.; Melia, Fulvio; Liu, Siming.

In: Astrophysical Journal, Vol. 555, No. 2 PART 2, 10.07.2001.

Research output: Contribution to journalArticle

Bromley, Benjamin C. ; Melia, Fulvio ; Liu, Siming. / Polarimetric imaging of the massive black hole at the galactic center. In: Astrophysical Journal. 2001 ; Vol. 555, No. 2 PART 2.
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