Bright Regions in Simeis 147
Click on the region for enhanced DSS images.
Simeis 147 is a gigantic supernova remnant in Taurus, comparable in apparent size to the Veil Nebula in Lyra, but much fainter. Steve Coe calls it "the Veil in a 2-inch scope." Although it's usually easier to detect faint deep sky objects if you know exactly where to look, you never know what you might find by sweeping the area ESE of Beta Tauri, the northern horn of the bull. Based upon the observing reports, you may wish to begin with Regions A & B
Region A ~05 40 +26 58
The first area observed was around star
Two arcs, one at SAO 77322, the other about 15' south were easily [!] visible. Much like the Veil, the arcs could be followed for approximately two degrees around the periphery of the
object. - Gil Shillcutt
Region B ~05 45 +27 03
The most amazing and intricate region of the entire SNR, this is an interwoven tapestry of filaments and nebulous arcs against a beautiful starry background. In one sector, several
filaments were visible criss-crossing each other at nearly right angles! - Rich Jakiel.
Region C ~05 39 +29 07
Thin trail of wisps and tendrils running ENE - WSW between
Faint nebulous arcs and patches were visible in regions 'D' and 'C'. Around C, some secondary details were visible, though not nearly as richly complex as in region B. - Rich
Jakiel
Region D ~05 43 +28 17
Nebulous patch about 30' SE of
A "clump" of ~8-12 sparse stars of ~10th magnitude and fainter ~10' in diameter was easily visible, resembling an OC of sorts. Faint hints of nebulosity were apparent surrounding the
entire "clump". When the scope was moved ~1 fov in the N/S direction, the nebulosity became a diffuse glow with definite edges some 10'x15' in size and oriented in an E/W direction. Averted
vision was not continuously required for this. - Jay McNeil
