Talk:Initial mass function: Difference between revisions
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{{WPAstronomy|object=|class=start|importance=Mid}} |
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{{physics|class=start|importance=low}} |
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The IMF exponent seemingly varies, according to galaxy type, from about 1.5 in lower mass galaxies, to nearly 3.0 in massive ellipticals. Popular references, referring to the original journal article: |
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http://www.sciencedaily.com/releases/2012/05/120501211411.htm |
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http://beforeitsnews.com/space/2012/04/under-dark-halo-old-galaxies-have-many-more-stars-2076436.html |
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[[Special:Contributions/66.235.38.214|66.235.38.214]] ([[User talk:66.235.38.214|talk]]) 04:38, 10 November 2012 (UTC) |
Revision as of 04:38, 10 November 2012
Astronomy Start‑class Mid‑importance | ||||||||||
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Physics Start‑class Low‑importance | ||||||||||
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The IMF exponent seemingly varies, according to galaxy type, from about 1.5 in lower mass galaxies, to nearly 3.0 in massive ellipticals. Popular references, referring to the original journal article:
http://www.sciencedaily.com/releases/2012/05/120501211411.htm http://beforeitsnews.com/space/2012/04/under-dark-halo-old-galaxies-have-many-more-stars-2076436.html
66.235.38.214 (talk) 04:38, 10 November 2012 (UTC)