The 'thick' radio disk of NGC 4565

Details The 'thick' radio disk of NGC 4565 The 'thick' radio disk of NGC 4565

Dec 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...153..281b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 153, no. 1, Dec. 1985, p. 281-283.

Astronomy and Astrophysics

Astrophysics

13

Emission Spectra, Galactic Cosmic Rays, Radio Observation, Spiral Galaxies, Flux Density, Signal To Noise Ratios

Scientific paper

A study of the radio continuum emission at 1414 MHz from the edge-on spiral galaxy NGC 4565 is presented. The results show the presence of an unresolved central source of 1.3 + or - 0.3 mJy and of a moderately bright disk with a possible two-component structure consisting of a thin disk and a thick one. These observations strongly support the view that radio disks of spiral galaxies are extended in the z-direction and may have a two-component structure. Also, a strict lower limit for the inclination angle of NGC 4565 is derived.

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