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