A Radio Survey of Bright Galaxies |
From inside the book
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Page 39
... cm neutral hydrogen line in absorption against the BSO at Arecibo , but was unsuccess- ful due to confusing emission ... cm line system is operational . Arp and ment should be repeated when the Arecibo 21 - cm interferometer or the VLA ...
... cm neutral hydrogen line in absorption against the BSO at Arecibo , but was unsuccess- ful due to confusing emission ... cm line system is operational . Arp and ment should be repeated when the Arecibo 21 - cm interferometer or the VLA ...
Page 52
... cm emission of neutral hydrogen in ellipticals ( Shostak et al . , 1975 , Huchtmeier et al . , 1975 , Bottenelli and Gouguenheim 1977 , Huchtmeier et al . , 1977 , Knapp , Gallagher and Faber 1978 , Knapp , Kerr , and Williams 1978 ) ...
... cm emission of neutral hydrogen in ellipticals ( Shostak et al . , 1975 , Huchtmeier et al . , 1975 , Bottenelli and Gouguenheim 1977 , Huchtmeier et al . , 1977 , Knapp , Gallagher and Faber 1978 , Knapp , Kerr , and Williams 1978 ) ...
Page 142
... cm line emission in elliptical galaxies with compact continuum sources , and to search for compact sources in the few ellipticals known to have HI emission , to see if the correlation implied by a small amount of data actually exists ...
... cm line emission in elliptical galaxies with compact continuum sources , and to search for compact sources in the few ellipticals known to have HI emission , to see if the correlation implied by a small amount of data actually exists ...
Contents
VII | 2 |
ACCURATE OPTICAL POSITIONS OF BRIGHT GALAXIES | 6 |
THE ARECIBO 2380 MHz SURVEY OF BRIGHT GALAXIES | 13 |
6 other sections not shown
Common terms and phrases
Abscissa apparent Arecibo survey Astr Bright Galaxies Catalog CHAPTER cluster ellipticals compact sources compared complete sample components CONF confusion consistent corrected dependence detected determined diameter difference disk distribution effect Ekers elliptical and lenticular elliptical galaxies errors expected extended sources field Figure flux densities fraction frequency gain galactic given greater higher Hubble type indicated interaction intrinsic lenticular galaxies less limit luminosity functions measured median nearly NGC MJY NGC RA Nilson noise normal nucleus objects observed occur optical luminosity pairs peak photographic magnitudes PLATE COORDINATES UGC pointing positions possible powerful prints probability produce radio emission radio luminosity radio sources radio to optical range ratio region resolved result scans shown similar space spectral spiral galaxies stars statistically strong supernova Table thermal tidal tion typical Uppsala W/Hz Zwicky clusters