MMT Hypervelocity Star Survey. II. Five New Unbound Stars

MOCCA Code for Star Cluster Simulations - II. Comparison with N-body Simulations

Model of the polarized foreground diffuse Galactic emissions from 33 to 353 GHz

Model-Independent Diagnostics of Highly Reddened Milky Way Star Clusters: Age Calibration

Modeling CO Emission: I. CO as a Column Density Tracer and the X-Factor in Molecular Clouds

Modeling CO Emission: II. The Physical Characteristics that Determine the X factor in Galactic Molecular Clouds

Modeling High-Mass Star Formation and Ultracompact HII Regions

Modeling Mid-Infrared Variability of Circumstellar Disks with Non-Axisymmetric Structure

Modeling molecular hyperfine line emission

Modeling of the Vela complex including the Vela supernova remnant, the binary system gamma2 Velorum, and the Gum nebula

Modeling proper motions beyond the Galactic bulge

Modeling Star counts in the Monoceros stream and the Galactic anti-centre

Modeling the dust emission from PN IC418

Modeling the effects of dust evolution on the SEDs of galaxies of different morphological type

Modeling the Galactic Magnetic Field using Rotation Measure Observations in the Galactic Disk from the CGPS, SGPS, and the VLA

Modeling the host galaxies of long-duration gamma-ray bursts

Modeling the Magnetic Field in the Galactic Disk using New Rotation Measure Observations from the Very Large Array

Modeling the Metallicity Distribution of Globular Clusters

Modeling the Newtonian Dynamics for Rotation Curve Analysis of Thin-Disk Galaxies

Modelling chemical abundance anticorrelations on globular cluster spectra