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Date and Time of the Query: 2019-06-25 T17:59:01 PDT
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For refcode 1988PASP..100..452T:
Retrieve 119 NED objects in this reference.
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Copyright by Astronomical Society of the Pacific. Reproduced by permission
1988PASP..100..452T CONTINUUM RADIO EMISSION FROM VIRGO GALAXIES KENNETH C. TURNER National Astronomy and Ionosphere Center, Arecibo Observatory, P.O. Box 995, Arecibo, Puerto Rico 00612 GEORGE HELOU Infrared Processing and Analysis Center, Caltech, 100-22, Pasadena, California 91125 AND YERVANT TERZIAN National Astronomy and Ionosphere Center, Cornell University, Ithaca, New York 14853 Received 1987 November 11, revised 1988 January 23 ABSTRACT We present 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). We also present interferometric measurements at the same frequency for 48 galaxies with <= 1 arc sec resolution. We discuss the relative concentration of the radio emission for these galaxies, particularly the emission from the galactic disk compared with that from the nucleus. It is found that the disk emission dominates in most cases. We also find some indications that the flux concentration is greater in elliptical and lenticular galaxies than it is in spirals. Key words: galaxies-radio emission
Retrieve 119 NED objects in this reference.
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