Rapid Optical Variability of the Source PKS 1514-24

Details Rapid Optical Variability of the Source PKS 1514-24 Rapid Optical Variability of the Source PKS 1514-24

Jul 1971

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1971natur.232..178b&link_type=abstract

Nature, Volume 232, Issue 5307, pp. 178-179 (1971).

Physics

32

Scientific paper

THERE are two cases in which radio sources have been identified with optical objects previously known as variable stars: the Seyfert galaxy 3C120 with the star BW Tau (ref. 1) and VRO 42 22 01 with BL Lac (ref. 2). As a systematic search for possible new concidences, 807 variable stars were selected from the General Catalog of Variable Stars3 and its first supplement4 using the following criteria: (i) type given as irregular or unknown; (ii) no spectral type given; and (iii) galactic latitude |bI|>10°. This list was checked for coincidences against A Master List of Radio Sources5 and the fourth instalment of the Ohio survey6. Only two coincidences were found.

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