|The Pipe Nebula and environs captured
by the Wide Field Imager on the MPG/ESO 2.2-meter telescope at ESO's
La Silla Observatory
The Pipe Nebula is an interconnected series of dark
nebulae which appears as a sinuous rift in the star fields of Ophiuchus.
The blackest, central portion is shaped somewhat like an old-fashioned smoker's
pipe, but the whole structure extends from the region of the Rho
Ophiuchi Nebula and the Lagoon Nebula,
and takes in a number of dark nebulae, including Barnard 59 (at the western
tip of the Pipe, just south of NGC 6293), 65, 66, 67, 77, 244, and 256.
It lies at a distance of 600–700 light-years and spans about six light-years.
|Location of the Pipe (red circle)
AND STAR CLUSTERS