Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21532505m&link_type=abstract
American Astronomical Society, AAS Meeting #215, #325.05; Bulletin of the American Astronomical Society, Vol. 42, p.422
Astronomy and Astrophysics
Astronomy
Scientific paper
Cosmic parameters are now known with great precision, including the cosmic baryon fraction. We make an inventory of the baryonic and total mass in structures ranging from the smallest galaxies to rich clusters of galaxies. We find that the fraction of detected baryons deviates systematically from the cosmic baryon fraction as a function of mass. On the largest scales of clusters, most but not all of the expected baryons are detected, while in the smallest dwarf galaxies, fewer than 1% are detected. Clearly it would be good to discover where these missing baryons reside, and to understand the systematic variation with mass.
SSM gratefully acknowledges support from NSF grant AST0908370.
de Blok J. G. W.
McGaugh Stacy S.
Schombert James M.
Zagursky Matthew J.
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