Possible subjects for 327 MHz VLBI observations

Details Possible subjects for 327 MHz VLBI observations Possible subjects for 327 MHz VLBI observations

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pbeio..11...13w&link_type=abstract

Beijing Astronomical Observatory, Publications, Sept. 1988, p. 13-20. Research supported by the National Natural Science Foundat

Astronomy and Astrophysics

Astrophysics

1

Astrophysics, Very Long Base Interferometry, Centimeter Waves, Image Resolution, Radio Sources (Astronomy), Seyfert Galaxies

Scientific paper

The 327-MHz sensitivity and resolution parameters of various existing and proposed terrestrial VLBI networks are reviewed, and astrophysical objects which could be characterized using these arrays are identified. Particular attention is given to extragalactic sources to be searched for fine (less than 30 marcsec) structures, compact steep-spectrum radio sources, the prominent cores of strong radio sources with arcsec-scale structures, morphological variants of low-frequency variables, samples of strong radio sources, steep-spectrum cores in extended sources, compact components in Seyfert galaxies, flat-spectrum sources, and sources well studied by VLBI at cm wavelengths. Graphs and tables of numerical data are included.

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