NGC 1514 (PK 165-15.1)
Taurus
Penryn, California
November 2003
FS-128G (ag, ST-4)
ST-10XME LRGB 2 minutes each
The nucleus of NGC 1514 is a close coupled binary system which drives the
morphology of the ejected shells. The bright knots in the ejected shells
are moving at a much higher rate of expansion and have a different chemical
composition then the underlying areas of the nebula.