Fuor-like light-curve variations of Orion association stars

Details Fuor-like light-curve variations of Orion association stars Fuor-like light-curve variations of Orion association stars

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987afz....27..447p&link_type=abstract

Astrofizika (ISSN 0571-7132), vol. 27, Dec. 1987, p. 447-458. In Russian.

Astronomy and Astrophysics

Astronomy

11

Light Curve, Orion Constellation, Stellar Flares, Variable Stars, Stellar Color, Stellar Luminosity

Scientific paper

The results of observations of fuor-like Sugano and Chanal objects in the Orion association are given. The light curve, amplitude of flare and colour index are determined. It has been shown that the Sugano object is both an Orion variable and a flare star. The values of δ' and δ are of the same order as in the case of fuors. An assumption about the intensification of the outflow of matter with the same velocities in those objects is made. The luminosity of P Cyg before the flare is determined.

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