Continuum radio emission from Virgo galaxies

Details Continuum radio emission from Virgo galaxies Continuum radio emission from Virgo galaxies

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pasp..100..452t&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 100, April 1988, p. 452-457. Research supported by NASA

Astronomy and Astrophysics

Astronomy

3

Continuous Radiation, Galactic Radio Waves, Radio Astronomy, Virgo Galactic Cluster, Elliptical Galaxies, Radiant Flux Density, Radio Emission, Radio Interferometers, Spiral Galaxies

Scientific paper

The paper presents single-antenna measurements of radio emission from 120 galaxies in the Virgo cluster at 2380 MHz using a 2.6 arc min beam (half-power beam width). It also presents interferometric measurements at the same frequency for 48 galaxies with less than or equal to 1 arc sec resolution. The relative concentration of the radio emission for these galaxies, particularly the emission from the galactic disk compared with that from the nucleus is discussed. It is found that the disk emission dominates in most cases. Some indications that the flux concentration is greater in elliptical and lenticular galaxies than it is in spirals are also found.

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