Photometry of the recurrent nova U SCO

Details Photometry of the recurrent nova U SCO Photometry of the recurrent nova U SCO

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992sval...18..201b&link_type=abstract

Soviet Astronomy Letters, Vol. 18, p. 201; Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 18, no. 6, June 1992, p. 505

Astronomy and Astrophysics

Astronomy

2

Light Curve, Novae, Stellar Rotation, Stellar Spectrophotometry, White Dwarf Stars, Stellar Luminosity, Stellar Magnitude, Ubv Spectra

Scientific paper

Photometric observations of U Sco were carried out during the 1987
outburst. The light curve is plotted on the basis of published data and
the present photometry. Light variations with a period of about 80 min,
caused by the axial rotation of the white dwarf, is suspected.

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