The Halo from the Outside In: QSO Absorption Lines

Details The Halo from the Outside In: QSO Absorption Lines The Halo from the Outside In: QSO Absorption Lines

Apr 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aspc...92..501c&link_type=abstract

Formation of the Galactic Halo...Inside and Out, ASP Conference Series, Vol. 92, 1996, Heather Morrison and Ata Sarajedini, eds.

Computer Science

1

Scientific paper

Studies of high resolution quasar absorption lines (QALs), arising from gas in local and z <= 1.5 galaxies, provide direct probes of the kinematic, chemical, and ionization conditions and evolution of Milky Way--like galaxies. Inferences drawn from these studies provide a powerful analog for those based upon direct studies of the halo. The observed gas kinematics and velocity evolution reveal that galactic halos are complex dynamical components, consistent with Searle--Zinn formation scenarios.

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