Photometric behavior of the subfuor V1118 ORI

Details Photometric behavior of the subfuor V1118 ORI Photometric behavior of the subfuor V1118 ORI

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992sval...18..248p&link_type=abstract

Soviet Astronomy Letters, Vol. 18, p. 248; Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 18, no. 7, July 1992, p. 619

Astronomy and Astrophysics

Astronomy

2

Light Curve, Stellar Flares, Stellar Spectrophotometry, Ubv Spectra, Variable Stars, Stellar Luminosity, Stellar Spectra

Scientific paper

Preliminary results of photometry of the subfuor V1118 Ori are presented. During a maximum the V1118 Ori object exhibits irregular rapid brightness oscillations, with an amplitude sometimes greater than one solar magnitude. V1118 Ori is characterized by excess UV emission and, on the two-color diagram (U-B)-(B-V), is in a region typical of T Tau type stars with a large UV excess.

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