
Tadpole Nebula
The Tadpole Nebula (IC 410) is an Ha region in the constellation Auriga about 12,400 light years away. It is associated with the young star cluster NGC 1893 at the center of the nebula. Tadpole...
The Tadpole Nebula (IC 410) is an Ha region in the constellation Auriga about 12,400 light years away. It is associated with the young star cluster NGC 1893 at the center of the nebula. Tadpole...
The Whirlpool Galaxy (M51) is an interacting grand design spiral galaxy in the constellation Canes Venatici about 31 million light years away. It is colliding with its companion, NGC 5195. M51 ...
The Whale Galaxy (NGC 4631) and the Hockey Stick Galaxy (NGC 4656) are barred spiral galaxies in the constellation Canes Venatici about 30 million light years away. Whale and Hockey Stick Gala...
The Cosmic Bat nebula (NGC 1788) is a nebula in the constellation of Orion. It has a wonderful mix of reflection nebula, dark nebula, and Ha throughout. NGC 1788 Gear Telescope...
The Flaming Star Nebula (IC 405) is a bright emission nebula in the constellation Auriga 1500 light years away. Flaming Star Nebula Gear Telescope PlaneWave Delta Rho 350...
IC 342, The Hidden Galaxy, is an active and bright galaxy obscured by dust from the Milky Way. The dust shifts the color from the galaxy towards the red and lowers its apparent brightness. IC 3...
NGC 7822, sometimes called the Question Mark Nebula, is a huge nebula so my field of view can only get a portion of it without resorting to a a mosaic. This image was the first time trying 10 minut...
This image started as a meme where the focus would be on M110 and you’d just ignore Andromeda over there in the corner. But after I started getting some data I was surprised at how much detail I wa...
This M33 image was first light for my new remote observatory located in south east Arizona. Several friends and I went to the observatory in mid October to install equipment and hopefully get some ...
The OIII “flower”, as some have come to call it, is an extremely faint OIII structure that is only visible after considerable integration and careful continuum subtraction. After 25.5 hours of OIII...