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IC 2006
Radio Astronom1y G
Overview on Spectral Line Source Finding and Visualisation
Atlas Menor Was Objects to Slowly Change Over Time
Resolving the AGN and Host Emission in the Mid-Infrared Using A
Extended H I Disks in Dust–Lane Elliptical Galaxies1
190 Index of Names
Super-Massive Black Hole Scaling Relations and Peculiar Ringed Galaxies
The Carnegie-Irvine Galaxy Survey. Iii. the Three-Component Structure of Nearby Elliptical Galaxies
ASEM Newsletter December2015
National Radio Astronomy Observatory Observing
1991Apj. . .379. .177L the Astrophysical Journal, 379:177-215
Southern Arp - Constellation
Arxiv:Astro-Ph/0004095V1 6 Apr 2000
Distribution of Slow and Fast Rotators in the Fornax Cluster
Eridanus Fluss Eridanus
Differences Between CO- and Calcium Triplet-Derived Velocity Dispersions in Spiral Galaxies: Evidence for Central Star Formation?
The ATLAS3D Project – XIV. the Extent and Kinematics of the Molecular Gas in Early-Type Galaxies
Depleted Cores, Multi-Component Fits, and Structural Parameter Relations
Top View
Arxiv:1806.06350V1 [Astro-Ph.GA] 17 Jun 2018 the Galaxy Population
Galaxy Morphology
Southern Arp - Declination
TABLE 4: Properties of Bars
Revised Shapley Ames.Pdf
Overview on Spectral Line Source Finding and Visualisation
Kinematical and Spatial Lopsidedness in Spiral Galaxies
Appendix: Swift's Deep Sky Catalogs
The Stellar Populations of Early-Type Galaxies in the Fornax Cluster
University of Groningen Spatial and Kinematical Lopsidedness of Atomic
Made-To-Measure Particle Models of Intermediate-Luminosity Elliptical Galaxies: Regularization, Parameter Estimation, and the Dark Halo of NGC 4494
Overview on Spectral Line Source Finding and Visualisation
December 10 2016 7:00Pm at the Herrett Center for Arts & Science Colleagues, College of Southern Idaho
TABLE 1 Explanation of CVRHS Symbolsa
Studies on the Composition, Distribution and Detection of Dark Matter in the Universe
Distribution of Slow and Fast Rotators in the Fornax Cluster
IC Catalogue Final.Xlsx
Measuring Infrared Surfacebrightness Fluctuation Distances with HST WFC3: Calibration and Advice
The Carnegie-Irvine Galaxy Survey. VIII. Demographics of Bulges Along the Hubble Sequence
The ACS Fornax Cluster Survey. I. Introduction to the Survey and Data
2MASS, See Two Micron All-Sky Survey Accretion Rings, 80 Active
MEASURING DISTANCES and PROBING the UNRESOLVED STELLAR POPULATIONS of GALAXIES USING INFRARED SURFACE BRIGHTNESS FLUCTUATIONS1 Joseph B
Ellipticity of Galaxies in Fornax Cluster Toon-Yarat Rattanaprapa Pua
The Ages of Elliptical Galaxies from Infrared Spectral Energy Distributions
Catalogue of One Thousand Galaxies