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Enriched haloes at redshift $z=2$ with no star-formation: Implications for accretion and wind scenarios
galaxies:evolution galaxies:formation galaxies:high-redshifts galaxies
2011/10/13
In order to understand which process (e.g. galactic winds, cold accretion) is responsible for the cool (T~10^4 K) halo gas around galaxies, we embarked on a program to study the star-formation propert...
Orbital Dynamics Analysis of Binary Systems in Mass-Loss Scenarios
Orbital Dynamics Analysis Binary Systems Mass-Loss Scenarios
2009/6/16
Orbital Dynamics Analysis of Binary Systems in Mass-Loss Scenarios。