The nature of the sources in the BG 408 MHz survey of the galactic plane

Details The nature of the sources in the BG 408 MHz survey of the galactic plane The nature of the sources in the BG 408 MHz survey of the galactic plane

May 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974mmsai..45..281f&link_type=abstract

(Ministero della Pubblica Istruzione, CNR, and Universita di Trieste, European Regional Meeting in Astronomy, 2nd, Trieste, Ital

Astronomy and Astrophysics

Astronomy

Galactic Radiation, Microwave Emission, Point Sources, Radio Sources (Astronomy), Galactic Structure, Monte Carlo Method, Spatial Distribution, Statistical Analysis, Supernovae, Thermal Radiation

Scientific paper

Observational data from a 408-MHz survey of radio sources in the galactic plane are statistically examined, with particular emphasis on discrimination between galactic and extragalactic sources. The survey was carried out using the East-West arm of the Bologna radio telescope in the region of 15 to 245 deg longitude and not more than 4 deg latitude. Arguments on the nature of particular sources are based on statistical interpretations of source counts, spatial distribution, spectral indices, and diameter distributions.

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