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Evolution of the IGM/Galaxy Halo Interface to z=2

Evolution of the IGM/Galaxy Halo Interface to z=2. Chris Churchill (New Mexico State University) Wal Sargent (Caltech) Michael Rauch (Carnegie). Evolution of the IGM/Galaxy Interface to z=2. Abstract.

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295 views • 12 slides

A Statistical Study of Mg II Absorption-Selected Galaxies in the SDSS at 0.3<z<0.5

A Statistical Study of Mg II Absorption-Selected Galaxies in the SDSS at 0.3<z<0.5. Brittney Curtis Astronomy 3350 Professor Donald Terndrup Ohio State University. (Credit: NASA; ESA; A. Feild , STScI ). We can use quasars to learn about the circumgalactic medium.

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250 views • 12 slides

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Mgii absorbers - PowerPoint PPT Presentation

Evolution of the IGM/Galaxy Halo Interface to z=2

A Statistical Study of Mg II Absorption-Selected Galaxies in the SDSS at 0.3&lt;z&lt;0.5

A Statistical Study of Mg II Absorption-Selected Galaxies in the SDSS at 0.3<z<0.5