Structure of the galactic background

Details Structure of the galactic background Structure of the galactic background

Apr 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975sva....18..543v&link_type=abstract

(Astronomicheskii Zhurnal, vol. 51, Sept.-Oct. 1974, p. 922-926.) Soviet Astronomy, vol. 18, Mar.-Apr. 1975, p. 543-545. Transl

Astronomy and Astrophysics

Astronomy

Galactic Radiation, Galactic Structure, Milky Way Galaxy, Radio Emission, Supernova Remnants, Astronomical Maps, Background Radiation, Interstellar Magnetic Fields, Isophotes, Stellar Envelopes

Scientific paper

Some problems concerning the interpretation of high-latitude galactic radiation and the nature of galactic loops are discussed. The assumption is made that, if Loop I is the remnant of a near supernova, then some phenomena should be observed which are caused by the effect of a local region of an ordered magnetic field on the expansion of the supernova envelope. The isophotes of Yates (1968) are discussed from this viewpoint.

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