Magnetic reconnection in emission nebulae in clusters of galaxies

Details Magnetic reconnection in emission nebulae in clusters of galaxies Magnetic reconnection in emission nebulae in clusters of galaxies

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ppcn.conf..395j&link_type=abstract

In ESA, Fourth International Toki Conference on Plasma Physics and Controlled Nuclear Fusion p 395-398 (SEE N94-22624 05-75)

Astronomy and Astrophysics

Astrophysics

Cooling Flows (Astrophysics), Emission Spectra, Galactic Clusters, Interplanetary Magnetic Fields, Magnetic Field Reconnection, Nebulae, Light (Visible Radiation), Line Spectra, Magnetic Field Configurations, Plasma Spectra

Scientific paper

The effects of magnetic reconnection as a mechanism of excitation of filaments with optical emission lines observed in cooling flows in clusters of galaxies are studied. Hydrodynamical time dependent calculations to follow the evolution of cooling condensations until the phase of optical line emission are used. The results indicate that a much better agreement with observational results of emission line intensities and line ratios is attained when an active participation of the magnetic field through reconnection is included.

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