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[APML] Re: M13 star colors



Hi Tony,

Interesting image because I believe that it is generally accepted by the scientific community that, with a few exceptions, the stars that make up globular clusters are nearly all "Population II" stars.  Population II stars are very old with very little metal content, were formed very early in the history of the universe and have typical ages believed to be in the range of 11 to 13 billion years old [some estimates range from 9 to 13 billion years].  Stars that populate globular clusters are typically pale yellow to orange and red in color with temperatures of 2700 Kelvins for the pale yellow ones [give or take a few degrees].  The orange and red ones are even cooler.

Thus, one would not expect to see a large population of blue stars in any globular cluster because all Type O and B stars that may have been in globular clusters have long since evolved to white dwarfs, a Type II supernova that leaves a neutron star, or a Type II supernova that leaves a black hole.  The main sequence life spans for Type O and B stars are believed to range from 1 million to 10 million years with no indication that new stars have formed in globular clusters over the last few billion years.

Check out:

http://www.aao.gov.au/images/captions/aat089.html

and

http://www.aao.gov.au/images/captions/aat076.html

Also check out:

http://www.seds.org/messier/glob.html


Best Regards,

Dean Jacobsen
www.astrophoto.net

At 05:56 PM 6/11/2002 -0700, you wrote:
Hi Folks,
 
   ...snip...   I used my usual reduction techniques and PS for image extraction from the 16 bit data... what I found was beautiful and dare I say it, scientifically significant... the stars really showed their colors. There are two main types... blue, and yellow-orange. Here and there some very red stars are visible... very old carbon stars? At any rate, not your usual M-13 shot.
 
      http://www.astrophoto.com/M13CCD.htm
 
     Have a good one,
 
           Tony