4 citations · 4 across the 1 of their papers we have counts for
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Halo Mergers, Galaxy Mergers, and Why Hubble Type Depends on Mass
Ariyeh H. Maller
In the CDM cosmological framework structures grow from merging with smaller structures. Merging should have observable effects on galaxies including destroying disks and creating s…
Intrinsic Properties of Low-z SDSS Galaxies
Ariyeh H. Maller, Andreas A. Berlind, Michael Blanton +1
Galaxies are seen from different viewing angles and their observed properties change as a function of viewing angle. In many circumstances we would rather know the intrinsic proper…
Simulating the Gaseous Halos of Galaxies
Tobias Kaufmann, James S. Bullock, Ari Maller +1
Observations of local X-ray absorbers, high-velocity clouds, and distant quasar absorption line systems suggest that a significant fraction of baryons may reside in multi-phase, lo…
Structure of Bright 2MASS Galaxies: 2D Fits to the Ks-band Surface Brightness Profiles
Daniel H. McIntosh, Ari H. Maller, Neal Katz +1
The unprecedented sky coverage and photometric uniformity of the Two Micron All Sky Survey (2MASS) provides a rich resource for obtaining a detailed understanding of the galaxies p…
Damped Ly-alpha Systems in Semi-Analytic Models: Sensitivity to dynamics, disk properties, and cosmology
Ariyeh H. Maller, Rachel S. Somerville, Jason X. Prochaska +1
Previously we have shown that it is possible to account for the kinematic properties of damped Lyman alpha systems (DLAS) in the context of semi-analytic models. In these models, h…
Optical Counterparts to Damped Lyman Alpha Systems
Ariyeh H. Maller, Jason X. Prochaska, Rachel S. Somerville +1
Previously we have shown (Maller et al, 1998) that the kinematics of Damped Lyman Alpha Systems (DLAS) as measured by Prochaska and Wolfe (1998) can be reproduced in a multiple dis…