These glowing areas of gas often contain the youngest stars in our galaxy as
well as some of the most fanciful images available to the astrophotgrapher.
Reflection Nebula are blue or white, while emission nebula are Normally
Red or green. While emission and reflection nebula normally contain young hot
stars, Planetary Nebulae are the result of stellar decrepitude. As most main
sequence stars age they often swell up into red giants, this process often
leaves the outer fringes of the stellar atmosphere free to escape. Also
matter is often thrown off the star by massive solar winds, The results of all
this mass is often ionized and its interaction with the magnetic fields as well
as the rotation of the star create small but very unique nebulae that vary from
small blue-green balls, to rings or rings within rings and other patterns
including hourglasses and just about anything else.
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M1 is a supernova remnant from a spectacular Supernova in
the year 1054. Records from almost every culture including possibly American
Indians living in the Southwest indicate that eh star was the brightest
thing in the sky for many weeks and was even visible in the daytime. While
it bears the popular designation of Messier 1, It was observed 1741 by John
Bevis. Messier acknowledged this in a letter in 1771. Charles Messier
observed this object in 1758 and is his first object of nuisance
nebula or objects that interfered with his job and that was to search for
comets.
This color composite is an LRGB image taken with a C-14
operating at f7 and a ST-10 Binned 3x3. |
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| M27 is also known as the Dumbbell Nebula. In a small
telescope visual observers truly do see a dumbbell shape. This full color
LRGB version taken with a C-14 and ST-10 at f7 and binned 3x3 shows,
not only the dumbbell shape, but the intricate colors of ionized oxygen
(blue-green) and red (ionized Hydrogen). This is large planetary
nebula |
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| M57 is the famous ring nebula. It is an ovalish
planetary nebula with a distinct central star. The nebula is seen as a very
dim smoke ring in smaller scopes. Larger scopes with high magnification will
present the central star and allow for observing the detail in the ring.
Taken with a C-14 at f7 and ST-10, LRGB CCD Stack and Astrodon filters |
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| The Trifid nebulas M-20 is a small nebula in the
constellation of Sagittarius. It mist prominent characteristics are the dark
shadows that separates it into3 ares and its unique color comobination of
Emission and Reflection nebula (red and Blue Colrs). This B&W image was
taken at the Texas Star Party Several years ago with an ST-7, AP 5 inch
refractor and G-11 mount. |
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| The Flame (NGC 2024) and Horse head (IC434 and B33) nebulae
are shown in color. This picture highlights
another type of Nebula, a dark one. The Horse head protruding into the Red
Emission nebula as well as the black ledge are all a large dark nebula. This
is a dense area of dust and gas that attenuate visible light. This is an
attempt by me to concentrate on the art and science of CCD astronomical
imaging for artistic reasons. This image was taken with a STL-4020, Astro
Don Filters, and a Takahashi FSQ 106N on an AP900 mount. THE LRGB Subframes
were stacked in CCD Stack and the color combine accomplished in Photoshop
with a slight color saturation adjust to bring out the colors. |
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| IC-405, the flaming star Nebula in H Alpha. This an total of
1.5 hour image of the nebula with the STL-4020 and the FSQ106. The wide
field give this nebula a different than "nominal" appearance |
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| The California nebula or NGC1499 in Perseus is a large Emission Nebula
similar to the red nebula behind the horsehead. It distinctive shape vaguely
resembles California, thus the moniker. This is a very large nebula, the
image only show about 60 percent of it. It is 1.5 in Hydrogen Alpha with the
STL-4020 and TAK FSQ106. |
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| The Rosette Nebulae in Monoceros surrounds the bright open
cluster NGC 2239. This is a 2 hour image with a TAK FSq106 and ST-10 in H
alpha. |
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| The Cocoon Nebula is a small cloud of Ionized gas in the
Constellation of Cygnus. Wider field images of this nebula show and
impressive dark nebula that punctuated by the Cocoon at one end. this was
taken with an ST-10 and a C-14 at f7 |
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| The image to the right is a wide field shot of the Orion
Nebula (M42) the little separate nebula (M43) and the running man Nebula
(NGC1977). This image shows the wide field possible with the Tak fsq106 and
the STL-4020. The image is over 90 minutes on a side. The image is assembled
from 40minutes of L and 20 minutes of R G B . |
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| M42 This is a similar image to above taken on the previous
night and cropped. In this case since NGC 1977 is out of frame I did not
brighten the image as much. This kept more of the subtle colors in the
nebula The exposure times are similar |
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