The galactic halo
Galactic halo origin and evolution postulated from chemical evolution assuming stellar evolution details
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Galactic halo origin and evolution postulated from chemical evolution assuming stellar evolution details
Alpha recombination line emission from galactic center detected, discussing possible origins in continuum source or interstellar medium
IR luminosity of galactic nucleus from far IR observations, noting considerations favoring nonthermal model consisting of multiple sources
Galactic abundances and cosmic ray spectra by IMP-4 satellite, obtaining He ratio
Sounding rocket X ray survey of Cassiopeia region for supernova remnants and galactic source distribution
Galactic gamma rays from OSO-3 observations attributed to decay of neutral pions produced by cosmic rays interaction with interstellar gas nucleons
High energy galactic gamma rays photons, suggesting two-component cosmic ray source model
Galactic cosmic ray energy spectra of light and medium nuclei from IMP-4 satellite measurements, investigating L/M ratio
Low energy galactic cosmic radiation energy spectra and charge composition in 2-14 Z range by OGO-5, suggesting two component model for origin
Soft X ray background galactic absorption and intensity measurements indicating inverse relation to columnar atomic hydrogen density
Galactic center region gamma radiation observations, discussing intensities, energy spectrum and decay
Galactic soft X ray and subcosmic ray heating and ionizing of interstellar H I regions
Radioactive abundances and stable products in chronological model for galactic heavy element nucleosynthesis
Intensity and spectral shape of diffuse X ray emission by galactic disk from cosmic ray heating of interstellar hydrogen
Limit on line emission in X ray background at high galactic latitudes - rocket observation
Thermal electron density and cosmic ray flux in galactic radio emissions
Observations of galactic center radiation and possible point sources obtained by gamma ray telescope flown on three balloon flights
Mathematical model using Monte Carlo method for modulation of galactic protons by solar wind