NGC 1491 is a diffused nebula in Perseus with a mag 11 O6-type star BD +50°886 in its center . The radiation from this star is exciting the molecular gas causing the pinkish glow and also forming the bubble around it. The intense radiation is also eroding the gas clouds surrounding it. Above the image is the asteroid trail of Eris as seen through the red, green and blue filters.
Location & Date |
Backyard, Abbott Observatory - Nov 20&21, 2008 |
Telescope | TMB 130SS Refractor, F/7 on a Losmandy G11, Prime Focus, Image scale 1.68 arcsec/pixel |
Camera |
SBIG ST-2000XM w/CFW8, AO8 Astrodon Tru Balance Filters CCD temp -15°C |
Exposure Times | (Ha) 18 x 10, (R) 6 x 10, (G) 6 x 10,(B) 4 x 10 Minutes, Bin 1x1 |
Other Information |
Image acquisition/focus/guiding/dither - CCD Autopilot V4 w/CCDSoft Focus - Moonlite Motorfocus w/FocusMax |
Image Processing |
* Images Plus 3.75beta 2 - Calibration, Normalize, Grading, Alignment, Normalized Average Combine, R/L Deconvolution, N/R, mild DDP * Adobe CS - RGB blend into Ha, Levels, Curves, Sharpening, Cropping, NR, JPEG conversion |