Titlebook: Galaxies and their Masks; A Conference in Hono David L. Block,Kenneth C. Freeman,Ivanio Puerari Conference proceedings 2010 Springer Scienc

預防注射

捐助

Super Star Clusters and Supernovae in Interacting LIRGs Unmasked by NIR Adaptive Optics,rived SN rates used for providing an independent measurement of the SF history of the Universe. We also present thus far the first NIR luminosity functions of super star cluster (SSC) candidates. The LFs can then be used to constrain the formation and evolution of SSCs via constraints based on initial mass functions and cluster disruption models.

抗體

inveigh

Brain-Imaging

Twin Masks of Spiral Structure? A Local Perspective,metry of the Galaxy’s spiral arms, often with conflicting results. While a general consensus exists that a global pattern exists, considerable disagreement remains in the details. Arm geometries, orientations, and even the number of arms are still debated. Close examination of the literature reveals

Insul島

完成才會征服

Range-Of-Motion

忙碌

Molecular Gas Properties of Galaxies: The SMA CO(2-1) B0DEGA Legacy Project,ogies in the circumnuclear regions. While in samples of “normal” galaxies the molecular gas does not seem to peak toward the nuclear regions for about 50% of the galaxies, barred galaxies and mergers show larger concentrations. However, we do not exactly know from an observational point of view how

neuron

,The DiVA’s Mask: Iconifying Galaxies and Revealing HI Anomalies,ibution and velocity behaviour of HI emission using the 3-D information in data cubes. We explore creating 3-D masks from model galaxy cubes generated using parameters determined by GalAPAGOS. We call our technique of applying these masks to the original HI data cubes, and subsequent analysis of the