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The IGM/Galaxy Connection - The Distribution of Baryons at z=0 (Hardcover, 2003 ed.)
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The IGM/Galaxy Connection - The Distribution of Baryons at z=0 (Hardcover, 2003 ed.)
Series: Astrophysics and Space Science Library, 281
Expected to ship within 10 - 15 working days
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This volume contains the proceedings of the meeting entitled, "The
IGM/Galaxy Connection: The Distribution of Baryons at z = 0. " The
meeting was held August 8 -10 at the National Center for
Atmospheric Research (NCAR) located in Boulder, Colorado on the
foothills of the Rocky Mountains (see conference photo). We
organized this meeting because we felt it was time to address the
link between galaxies and the intergalactic medium at low redshift.
In this vein, we posed several questions to the conference
participants: Where are the baryons in the local universe and in
what phase do they reside? What signatures of galaxy evolution have
been imprinted on the IGM? What percentage of intergalactic gas is
left from the galaxy formation process? What does the distribution
of baryons at z = 0 tell us about the early universe? The
conference was an overwhelming success with lots of friendly
interaction and discussion among the participants. At lunch we were
treated to splendid views from the NCAR terrace and discussions
rang ing from the importance of the LSR, GSR, and LGSR velocity
frames to how long the desserts would last with 90 astronomers and
the hot Boul der sun. From an inventory of the baryons, to the
associations between galaxies and Lya absorbers, to the mechanisms
by which galaxies obtain and lose gas, the conference covered many
topics. The results of these endeavors are contained in these pages
and eloquently summarized by Chris Impey."
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