Weak Galactic radio sources and the spiral structure near the sun

Details Weak Galactic radio sources and the spiral structure near the sun Weak Galactic radio sources and the spiral structure near the sun

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986pazh...12..353p&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 12, May 1986, p. 353-360) Soviet Astronomy Letters (ISSN 0360-0327), vol. 12, May-June

Astronomy and Astrophysics

Astronomy

Galactic Structure, Radio Sources (Astronomy), Solar Neighborhood, Star Formation, Milky Way Galaxy, Stellar Luminosity

Scientific paper

For selected fields of the Milky Way in I and III quadrants of galactic longitudes the differential statistics of radio sources detected at 7.6 cm with RATAN-600 are compared. Nearly one half of the previously detected population of weak galactic radio sources consists of radio sources likely connected with star formation regions within (1 - 2) kpc from the sun. Probable luminosity of the sources is (30 - 50) mJy kpc2.

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