Windblown NGC 3199
Explanation:
NGC 3199 lies about 12,000 light-years away,
a glowing cosmic cloud in the southern constellation
of Carina.
The nebula is about 75 light-years across in this haunting,
false-color view.
Though the deep image reveals a more or less complete
ring shape, it does look very lopsided with a much brighter edge
at the lower right.
Near the center of the ring is a
Wolf-Rayet star, a massive, hot,
short-lived star that generates an intense stellar wind.
In fact, Wolf-Rayet stars are known to create nebulae
with
interesting
shapes as their powerful winds sweep
up surrounding
interstellar
material.
In this case, the bright edge was thought to indicate a
bow shock
produced as the star plowed through a uniform medium, like a boat
through water.
But
measurements
have shown the star is not really moving directly
toward the bright edge.
So a more likely explanation is that the
material surrounding the star is not uniform, but
clumped and denser near the bright edge of windblown NGC 3199.
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Authors & editors:
Robert Nemiroff
(MTU) &
Jerry Bonnell
(USRA)
NASA Web Site Statements, Warnings,
and Disclaimers
NASA Official: Jay Norris.
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rights apply.
A service of:
LHEA at
NASA /
GSFC
& Michigan Tech. U.
