Statistics on the symmetric magnetic fields in spiral galaxies

Details Statistics on the symmetric magnetic fields in spiral galaxies Statistics on the symmetric magnetic fields in spiral galaxies

Feb 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.200..313v&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 200, no. 2, p. 313-323.

Astronomy and Astrophysics

Astrophysics

3

Interstellar Magnetic Fields, Magnetic Field Configurations, Spiral Galaxies, Dynamo Theory, Hydrogen, Interstellar Gas, Statistical Analysis

Scientific paper

Updated magnetic data were used to reconsider preliminary correlations or results on agents including triggers, catalysts, and indicators of the magnetic field shapes. Results confirm two possible correlations: between magnetic field shape m(azim)(0, or 1) vs neutral H I gas mass (high 7 x 10 exp 9 solar masses, or low 1 x 10 exp 9 solar masses), and between m(azim)(0, or 1) vs neutral H I gas distortion or archness VA (low 1 to 2, or high 3 to 4).

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