V838 Mon: Radical spectral changes at short wavelengths

Astronomy and Astrophysics – Astronomy

Scientific paper

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Optical, Ultra-Violet, Binaries, Novae, Variables, Stars

Scientific paper

We continue multicolor photometric CCD UBVRI monitoring of the peculiar red nova V838 Mon using CCD photometer and SAO RAS 1-m reflector. New observations were obtained in two nights in October 2008. We noted strong changes in the U and B bands happened between 2008 April and October. The star became invisible in U band frames. Each night we have accumulated 6000 s exposures to get a measurable image of the star.

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