Romano's star in M33 - LBV candidate or LBV?

R. Kurtev; O. Sholukhova; J. Borissova; L. Georgiev

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Romano's star in M33 - LBV candidate or LBV?

R. Kurtev·O. Sholukhova·J. Borissova·L. Georgiev

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Abstract

We present the light curve of Luminous Blue Variable candidate star GR290 (Romano's star) in M33. The photographic photometry was made in photographic plates taken in B band of the M33 galaxy and cover an eight year period, 1982 - 1990. Twenty five plates, separated in seven groups, have been used. CCD B magnitude of the star is also presented. The analysis of our data together with the Romano's magnitudes (1978) shows "normal" eruptions with amplitude of more than 1 mag and timescale of about 20 years and smaller oscillations with amplitude 0.5 mag and a period of about 320 days. This is a typical photometrical behavior for LBVs.

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R. Kurtev, O. Sholukhova, J. Borissova, L. Georgiev. 2001-02-01. Romano's star in M33 - LBV candidate or LBV?. https://arxiv.org/abs/astro-ph/0102020

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