The bright spiral galaxy M106 (NGC 4258) in Ursa Major. This system
is distinguished by “anomalous arms”, better described perhaps as jets,
seen curving outward through the disk in radio emission and optical
emission lines. Recent measurements of maser regions near the nucleus
suggest a supermassive dark object (a black hole candidate with mass of
order 100 million solar masses)
at the center of this galaxy. This pseudocolor rendition was made from
a V-band CCD frame covering a region 9 arcminutes square, taken with the
1.1-meter Hall telescope of Lowell Observatory.
Credit: Bill Keel, University of Alabama.
- More images from Bill Keel’s collection
Details in the central region of M106
Image of M106 from an anonymous source.
- Amateur images of M106
- VLA radio investigations of M106
Last Modification: 25 May 1999, 14:00 MET