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SHELL GAME IN THE LMC (APOD 18May06)

Posted: Thu May 18, 2006 1:54 pm
by BMAONE23
Todays APDO

http://antwrp.gsfc.nasa.gov/apod/ap060518.html

shows that the Large Magellanic Cloud contains many nebula that are made of energetic hydrogen. It seems to be even more dramatic in black & white rather than in red.

The high resolution view is breath taking.

http://antwrp.gsfc.nasa.gov/apod/image/ ... ason_f.jpg

It makes me wonder what our galaxy would look like if photographed in this same manner. The LMC looks like it is wall to wall nebula.

Posted: Thu May 18, 2006 2:10 pm
by orin stepanek
I'd like to see the Milky way done in a like manner too. Also some of the other neighboring galaxies.
Orin

Posted: Fri May 19, 2006 7:44 am
by l3p3r
are there any false colour versions of this one floating about by any chance ?

Posted: Fri May 19, 2006 10:52 am
by makc
What's the problem with making one?

Image

Posted: Fri May 19, 2006 11:05 am
by harry
Hello All

I love the image, its amazing how many are popping up.

Are they Nova or supernova.

There seems to be both.

I assume this process is part of the recycle process.

Posted: Fri May 19, 2006 3:11 pm
by makc
orin stepanek wrote:I'd like to see the Milky way done in a like manner too.
search and find more.

Posted: Fri May 19, 2006 3:54 pm
by Qev
harry wrote:Are they Nova or supernova.

There seems to be both.
Primarily, these are H-II regions, which are nebulas containing young or newborn stars, where star formation is taking place. A good example of this in our galaxy is the Orion Nebula. The bubbles are being formed by the powerful stellar winds of hot, young stars blowing the material of the nebula away from them.

Posted: Fri May 19, 2006 9:59 pm
by harry
Hello qev

The size of the clouds would inidcate
either
Stellar winds
Dwarf nova
Nova
or supernova

What extent do stellar winds have?

Posted: Tue Jun 13, 2006 8:27 pm
by orin stepanek
http://antwrp.gsfc.nasa.gov/apod/ap060518.html
Has anyone noticed there seems to be some of the gas forming clouds that make a curved line through the center of the LMC? Not that it seems to have any significance; but is kind of a curious thing.
Orin

Posted: Wed Jun 14, 2006 8:10 am
by harry
Hello All

The Tarantula Nebula

http://antwrp.gsfc.nasa.gov/apod/ap060106.html
The spindly arms of the Tarantula Nebula surround NGC 2070, a cluster that contains some of the intrinsically brightest, most massive stars known. Intriguing details of the nebula's core can be seen in this remarkable skyscape, a composite of 31 hours of exposure time. This cosmic Tarantula also lies near the site of the closest recent supernova.

http://antwrp.gsfc.nasa.gov/apod/ap060518.html
Ionized by energetic starlight, a hydrogen atom emits the characteristic red H-alpha light as its single electron is recaptured and transitions to lower energy states. As a result, this image of the LMC seems covered with shell-shaped clouds of hydrogen gas surrounding massive, young stars. Sculpted by the strong stellar winds and ultraviolet radiation, the glowing hydrogen clouds are known as H II (ionized hydrogen) regions
.


So we do have mostly Nova and some supernova.