Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...396..686v&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 396, no. 2, Sept. 10, 1992, p. 686-695. Research supported by NSERC, Nation
Astronomy and Astrophysics
Astronomy
73
Electromagnetic Scattering, Electron Scattering, Galactic Nuclei, Infrared Stars, Interstellar Masers, Radiation Distribution, Angular Distribution, Hydroxyl Radicals, Line Spectra, Power Spectra, Stellar Envelopes, Very Long Base Interferometry
Scientific paper
Angular broadening measurements of 20 OH/IR stars near the Galactic center are reported. VLBA antennas and the VLA were employed to perform a MkII spectral line VLBI experiment. The distribution of interstellar scattering toward the Galactic center is determined on the basis of the present data, together with additional data taken from the literature. A region of pronounced scattering (525 mas at 1.612 GHz) nearly centered on Sgr A* was found. Two interpretations for the enhanced scattering are presented. One hypothesis is that the scattering is due to a clump of enhanced turbulence, such as those that lie along lines of sight to other known objects, that has no physical relationship to the Galactic center. The other model considers the location of the enhanced scattering to arise in the Galactic center itself. The physical implications of the models provide information on the nature of the interstellar scattering.
Cordes James M.
Diamond Philip J.
Frail Dale A.
van Langevelde Huib J.
No associations
LandOfFree
Interstellar scattering toward the Galactic center as probed OH/IR stars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Interstellar scattering toward the Galactic center as probed OH/IR stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Interstellar scattering toward the Galactic center as probed OH/IR stars will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1765968