Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987aj.....94.1178y&link_type=abstract
Astronomical Journal (ISSN 0004-6256), vol. 94, Nov. 1987, p. 1178-1184.
Astronomy and Astrophysics
Astronomy
112
Galactic Nuclei, Nonthermal Radiation, Radio Sources (Astronomy), Thermal Emission, Astronomical Maps, Field Strength, Ionization, Magnetic Fields, Point Sources
Scientific paper
Using a high-resolution radio-continuum image made at a frequency of 4.8 GHz, the authors discuss the radio source G0.18-0.04 located at the intersection of the galactic center Arc with the galactic plane. In this direction, the radio Arc is composed of a set of linear, nonthermal filamentary structures superimposed on a narrow, sickle-shaped, thermal feature which crosses them. The radio image suggests a physical interaction between the thermal and nonthermal structures. The authors argue that the magnetic field is dynamically important and estimate that its strength is very large, ≡10-3G. Furthermore, they suggest that the ionization of G0.18-0.04 is caused by collisional ionization rather than ultraviolet photons from massive stars. The discussion presents possible ways in which some of the energy of the relativistic particles or the magnetic field in the nonthermal filaments might be extracted to ionize ambient gas in the galactic plane.
Morris Mark
Yusef-Zadeh Farhad
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