Rapid strengthening of iron forbidden lines in the spectrum of V838 Mon

Details Rapid strengthening of iron forbidden lines in the spectrum of V838 Mon Rapid strengthening of iron forbidden lines in the spectrum of V838 Mon

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006atel..803....1b&link_type=abstract

The Astronomer's Telegram, #803

Astronomy and Astrophysics

Astrophysics

9

Optical, Binaries, Novae, Variables, Stars

Scientific paper

V838 Mon is a peculiar nova which showed a red K-M type spectrum in its outburst in 2002. Along with two similar objects, V4332 Sgr and M31 V1006/7, it forms a new class of eruptive variable stars. We report spectral observations obtained with the Russian 6-m BTA telescope (Special Astrophysical Observatory). In our spectrum taken on 2005 December 11 (3960-5741A, resolution 4.6A) two known companions of this binary system are seen, B3V star and cool oxygen-rich L type supergiant, the remnant of the outburst.

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