A multifrequency radio continuum survey of M33. I - Observations

Details A multifrequency radio continuum survey of M33. I - Observations A multifrequency radio continuum survey of M33. I - Observations

Feb 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26as...68..171b&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 68, no. 1, Feb. 1987, p. 171-185.

Astronomy and Astrophysics

Astrophysics

13

Radio Galaxies, Spiral Galaxies, Astronomical Maps, Continuous Radiation, Linear Polarization, Point Sources, Radiant Flux Density

Scientific paper

The authors present radio continuum surveys of M33 with the Effelsberg 100-m telescope at 21.1 cm, 17.4 cm, 11.1 cm, 6.3 cm and 2.8 cm. The data are displayed as distributions of total intensity and linear polarization. Thirty-eight point sources in a 2°×2° field around M33 are seen which are either constituents of the galaxy or background sources. A chain of up to nine sources may be connected with the known large-scale alignment of quasars and radio galaxies to the southwest of M33.

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