| Description |
V838 Mon is one of the most enigmatic objects observed in stellar
astrophysics in recent decades. It came to attention when it underwent
a powerful eruptive outburst in Jan. 2002, increasing in luminosity by a
factor of 100 over a period of 3 months. Immediately following this event
a spectacular light echo was formed from the outburst light reflecting off
the surrounding dust. Hubble Space Telescope images following this
expanding light echo have brought V838 Mon to public attention. What
makes V838 Mon an unusual star is that the outburst is not of any type
heretofore seen; the scenarios of a nova-like event or thermonuclear
runaway have been discounted, on the basis of the stellar type and
outburst details. The theories that best explain the outburst are a giant
star engulfing a planetary system or, more likely, a merger between a
very low mass star and a very young, maybe pre-main sequence
low-intermediate mass star.
Observations show that the envelope of the star expanded in response
to the stellar impact, and than it may now be beginning to contract. Many
O-bearing molecules, dust, an SiO maser and possibly a jet have been
observed from the star. If the outburst was indeed caused by the merging
of two stars, this is an extremely rare event. Herschel observations of
this star will allow us to model the kinematics, chemistry, temperature
and density structure of the stellar photosphere and the cool envelope
surrounding the star. These will help answer questions still remaining
about the stellar impact, and will also allow us to understand more about
how a star responds to such a violent event. |
