Dying SiO masers in the V407 Cyg system

Details Dying SiO masers in the V407 Cyg system Dying SiO masers in the V407 Cyg system

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2519....1d&link_type=abstract

The Astronomer's Telegram, #2519

Astronomy and Astrophysics

Astronomy

1

Radio

Scientific paper

The symbiotic nova, V407 Cyg, is a system having a Mira-type cool stellar component with circumstellar SiO maser emission (Deguchi et al. 2005; PASJ 57, 939). The nova outburst occurred in the V407 Cyg system can significantly influence the structure of the circumstellar shell of the cool star in a short time scale. We have been monitoring the time variation of SiO maser emission in the V407 Cyg system with the Nobeyama 45m telescope every few days since March 16, 2010.

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