Diffuse Baryons in the Universe: Galaxies, Warm Gas, or Cold Lonely Lumps

Details Diffuse Baryons in the Universe: Galaxies, Warm Gas, or Cold Lonely Lumps Diffuse Baryons in the Universe: Galaxies, Warm Gas, or Cold Lonely Lumps

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003assl..281...11b&link_type=abstract

The IGM/Galaxy Connection: The Distribution of Baryons at z=0, ASSL Conference Proceedings Vol. 281. Edited by Jessica L. Rosenb

Computer Science

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Scientific paper

It would seem that baryons are playing a clever game of hide and seek. Theorists tell us, almost precisely, how many baryons should be out there, but mere observers seem to have difficulty in locating the main baryonic repositories. While observations are necessarily imprecise, it does seem likely that the missing baryons are in some diffuse component (either cold or warm) that is simply very difficult to detect. In this contribution I will discuss the possible nature of this diffuse component and our ability to detect it.

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