Spectroscopic observations of the recurrent nova RS Ophiuchi from 1959 to 1968

Details Spectroscopic observations of the recurrent nova RS Ophiuchi from 1959 to 1968 Spectroscopic observations of the recurrent nova RS Ophiuchi from 1959 to 1968

Jan 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969cokon..65..257b&link_type=abstract

Communications of the Konkoly Observatory, No. 65 (Vol. VI, 1), p. 257-260 (1969)

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Scientific paper

Spectra of RS Oph have been taken at Asiago with the 122 cm telescope during the 1959-67 minimum and on the occasion of the 1967-68 outburst. At minimum the variable has a composite spectrum, one component being of spectral type around M2, while the other component gives a blue continuum with emission lines of medium or high excitation. during the outburst the star has shown the same spectral evolution as in the 1933 and 1958, with the development of bright nebular and coronal lines, indicating an extremely high degree of ionization. Further details will be given in a forthcoming paper.

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