Saturday, September 14, 2013

M27 The Dumbbell Nebula

From Wikipedia:

The Dumbbell Nebula (also known as Apple Core Nebula, Messier 27, M 27, or NGC 6853) is a planetary nebula in the constellation Vulpecula, at a distance of about 1,360 light years.
This object was the first planetary nebula to be discovered; by Charles Messier in 1764. At its brightness of visual magnitude 7.5 and its diameter of about 8 arcminutes, it is easily visible in binoculars, and a popular observing target in amateur telescopes.



SW254N
EQ-g
guided
Canon 350d (modified)
ISO800
15 each 2 min images
Darks, Flats, Bias applied

IC1396 The Elephants Trunk

I've finally had some decent weather. Few clouds and no wind. I had a chance to take an image of an object I've never taken before:


From Wikipedia:
The Elephant's Trunk nebula is a concentration of interstellar gas and dust within the much larger ionized gas region IC 1396 located in the constellation Cepheus about 2,400 light years away from Earth.[1] The piece of the nebula shown here is the dark, dense globule IC 1396A; it is commonly called the Elephant's Trunk nebula because of its appearance at visible light wavelengths, where there is a dark patch with a bright, sinuous rim. The bright rim is the surface of the dense cloud that is being illuminated and ionized by a very bright, massive star that is just to the west of IC 1396A. (In the Figure above, the massive star is just to the left of the edge of the image.) The entire IC 1396 region is ionized by the massive star, except for dense globules that can protect themselves from the star's harsh ultraviolet rays.
The Elephant's Trunk nebula is now thought to be a site of star formation, containing several very young (less than 100,000 yr) stars that were discovered in infrared images in 2003. Two older (but still young, a couple of million years, by the standards of stars, which live for billions of years) stars are present in a small, circular cavity in the head of the globule. Winds from these young stars may have emptied the cavity.
The combined action of the light from the massive star ionizing and compressing the rim of the cloud, and the wind from the young stars shifting gas from the center outward lead to very high compression in the Elephant's Trunk nebula. This pressure has triggered the current generation of protostars.[2]

SW254N

EQ-g

guided

Canon 350d (modified)

ISO800

15 each 2 min images

Darks, Flats, Bias applied

Friday, September 13, 2013

NGC6960 Veil Nebula (aka witches broom)

I finally got some clear sky and time combined so I took the opportunity to take the following image of the Veil Nebula.








SW254N
EQ-g
guided
Canon 350d (mod)
20 images at 2 mins each.
Darks, Flats and bias subtracted.