by Steve Gottlieb
I spent the early evening cleaning up the remaining NGC galaxies I had left in Antlia and Hydra and moved into Virgo and Coma when the seeing softened in the southwest. I didn't have a problem resolving SN 2004bd (coincidentally discovered on my birthday) from the core in my 18-inch Starmaster when the seeing was fairly steady. Here are two observations of the host galaxy, NGC 3786, 14 years apart. This same galaxy had another supernova just a couple of years back, so apparently it's quite active!
18" (4/10/04): moderately bright, fairly small, elongated 2:1 WSW-ENE, brighter core. Observed SN 2004bd, discovered less than a week earlier on 4/4/04 and situated just 4.7" W and 1.2" S of center. When the seeing steadied, the supernova was clearly resolved as a mag 14.5 "star" close WSW of the geometric center (along the major axis) and very close to the brighter core. Forms a pair with N3788 1.4' NE of center. A mag 10.8 star lies 2.0' SE.
17.5" (2/24/90): moderately bright, moderately large, elongated 5:2 WSW-ENE, bright core. Forms a pleasing close pair with N3788 (separation of 1.4' NE). The galaxies are elongated at nearly right angles and almost attached at the ENE end of N3786. A mag 10.5 star is 2' SE.
Posted on sf-bay-tac Apr 11, 2004 18:28:38 PT
Converted by report.pm 1.1 Jul 10, 2004 18:19:52 PT