The Far Ultraviolet Spectroscopic picture of the Missing Baryons in the Local Group

Details The Far Ultraviolet Spectroscopic picture of the Missing Baryons in the Local Group The Far Ultraviolet Spectroscopic picture of the Missing Baryons in the Local Group

2002-07-31

arxiv.org/abs/astro-ph/0208012v2

Astronomy and Astrophysics

Astrophysics

Accepted for publication in Nature, on December 4, 2002. To replace the original version submitted to Nature on May 13 2002, a

Scientific paper

The number of detected baryons in the low-redshift Universe (z < 1) is far small er than the corresponding number of baryons observed at higher redshift. According to hydrodynamical simulations for the formation of structure in the Universe, up to 2/3 of the 'missing baryons' may have escaped identification so far, due to their high temperature and low density. One of the few ways to detect this matter is to look for its UV absorption signature on the light from background sources. Here we show that the amplitude of the average velocity vector of 'high velocity' OVI absorbers detected in a UV survey of AGN decreases significantly in moving from the Local Standard of Rest, to the Galactic Standard of Rest and Local Group frames. At least 82 % of these absorbers are not associated with any 'high velocity' HI complex (HV-HI) in our Galaxy, and so are strongly implicated as being due to primordial Warm-Hot Intergalactic Medium (WHIM) pervading an extended Galactic Corona or our Local Group. We estimate that the total baryonic mass contained in this medium is as large as ~ 1e12 solar masses, similar to the combined mass of the two most massive virialized constituents of the Local Group (the Andromeda and the Milky Way galaxies), and of the order of the mass required to dynamically stabilize the Local Group.

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