Abstracts, Galactic Center Workshop '98
GCNEWS
A Newsletter for Galactic Center Research
This Volume was edited by Angela Cotera & Heino Falcke
email: gcnews@aoc.nrao.edu

ABSTRACT

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Life Time of the Radio Arc Filaments determined by mm-Wave Observations with the 100-m Telescope
Sofue, Y.1,2, Reich, W.1, Reich, P.1, & Wielebinski, R.1
1Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121, Bonn, Germany; 2Institute of Astronomy, The University of Tokyo, Mitaka, Tokyo 181-8588, Japan;
ABSTRACT:
High-resolution continuum mapping of the Radio Arc has been made
at 43 GHz using the Effelsberg 100-m telescope in order to
investigate spatial variation of the spectrum.
The straight nonthermal filaments, clearly seen at 32 GHz and
lower frequencies, are very weak at 43 GHz.
The spectral index of the brightest filaments, which is flat
at lower frequencies, turns to be as steep as alpha ~ -1
between 32 and 43 GHz, indicating
a spectral turnover between these frequencies.
Assuming that the magnetic field strength is ~ 1 mG, we estimate
the life time of cosmic-ray electrons to be several thousand years,
showing that the filaments are short-lived structures.
The present result would give a constraint on the location and
epoch as well as the initial energy distribution of
injected cosmic-ray electrons.
On the other hand, ``Sickle" is
clearly visible at 43 GHz and has a flat spectrum,
which confirms its thermal characteristics.
"Pistol" appears to show a peculiarly inverted spectrum,
suggesting a two-component spectrum.
LINKS: Program, Author, sofue@mtk.ioa.s.u-tokyo.ac.jp
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