Astronomy and Astrophysics – Astronomy
Scientific paper
May 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apj...304...82d&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 304, May 1, 1986, p. 82-95.
Astronomy and Astrophysics
Astronomy
31
Cosmic Rays, Radiation Sources, Radio Astronomy, Spiral Galaxies, Star Distribution, Charge Coupled Devices, Emission Spectra, Ionized Gases, Particle Production, Relativistic Particles, Visual Observation
Scientific paper
An observational technique is presented for addressing the problem of the origin of cosmic rays in galaxies by determining and comparing the distributions of cosmic rays, stars, and thermal gas. It is argued that optical continuum, emission line, and radio continuum imaging can be used to determine the distributions of the major stellar populations, the ionized gas, and the cosmic rays in galactic disks. An application of the technique is demonstrated by presenting and discussing observations of the spiral galaxy, NGC 3310. A preliminary analysis points to a possible spiral arm origin but argues against conventional models of cosmic-ray production such as supernova remnants.
Crane Patrick C.
Davis Lindsey Elspeth
Duric Neb
Seaquist Ernest R.
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