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Astrophysicists produce the first age map of the halo of the Milky Way     Astrophysicists  first age map  Milky Way       font style='font-size:12px;'> 2015/11/12
University of Notre Dame astronomer Timothy Beers and his Galactic Archaeology group, which includes Notre Dame astronomers Daniela Carollo and Vinicius Placco, have led an international team of resea...
We present imaging and spectroscopy of NGC 40 acquired using the Spitzer Space Telescope (Spitzer), and the Infrared Space observatory (ISO). These are used to investigate the nature of emission from ...
This is the second paper of a series that reports on our investigation of the clustering properties of AGNs in the ROSAT All-Sky Survey (RASS) through cross-correlation functions (CCFs) with Sloan Dig...
Using conditional luminosity functions (CLFs) which encode the luminosity distribution of galaxies as a function of halo mass, we construct a halo model of IRAS galaxies selected at 60 micron. An abun...
Anyone out there? Galactic Halo Post-AGB stars     Galactic Halo  Post-AGB stars       font style='font-size:12px;'> 2011/1/11
We present results of a survey of post-asymptotic giant branch stars (post-AGBs) at high galactic latitude. To date, few post-AGB stars are known throughout the Galaxy and the number of known members ...
The bispectrum vanishes for linear Gaussian elds and is thus a sensitive probe of non- linearities and non-Gaussianities in the cosmic density eld. Hence, a detection of the bispectrum in the halo ...
Large scale anisotropies on halo infall      large scale structures  overdensities  infall  statistical  haloes       font style='font-size:12px;'> 2010/11/15
We perform a statistical analysis of the peculiar velocity field around dark mat- ter haloes in numerical simulations. We examine different properties of the infall of material onto haloes and its r...
Physical Properties of Complex C Halo Clouds     rgalactic medium −   ISM  structure −   ISM       font style='font-size:12px;'> 2010/11/9
Observations from the Galactic Arecibo L-Band Feed Array HI (GALFA-HI)Survey of the tail of Complex C are presented and the halo clouds associated with this complex cataloged. The properties of the Co...
Linking haloes to galaxies: how many halo properties are needed?      galaxies  formation       font style='font-size:12px;'> 2010/11/15
Recent studies emphasize that an empirical relation between the stellar mass of galaxies and the mass of their host dark matter subhaloes can predict the clustering of galaxies and its evolution wit...
A Two-Point Correlation Function For Galactic Halo Stars      galaxies – Milky Way  formation       font style='font-size:12px;'> 2010/11/12
We describe a correlation function statistic that quantifies the amount of spatial and kinematic substructure in the stellar halo.We test this statistic using model stellar halo realizations construct...
We present and analyze the positions, distances, and radial velocities for over 4000 blue horizontal-branch (BHB) stars in the Milky Way's halo, drawn from SDSS DR8. We search for position-velocity su...
The Galactic halo magnetic field revisited     The Galactic halo  magnetic field        font style='font-size:12px;'> 2011/1/10
Recently, Sun et al. (2008) published new Galactic 3D-models of magnetic fields in the disk and halo of the Milky Way and the distribution of cosmic-ray electron density by taking into account the the...
Modelling the HI halo of the Milky Way     Galaxy Astrophysics (astro-ph.GA)       font style='font-size:12px;'> 2011/1/7
We studied the global distribution and kinematics of the extra-planar neutral gas in the Milky Way.
A longstanding puzzle of fundamental importance in modern cosmology has been the origin of the nearly universal density profiles of dark matter halos found in N-body simulations -- the so-called NFW p...
We investigate the possibility that Hercules, a recently discovered Milky Way (MW) satellite, is a stellar stream in the process of formation. This hypothesis is motivated by Hercules' highly elongate...

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