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Abell 383
Highlights and Discoveries from the Chandra X-Ray Observatory1
Stsci Newsletter: 2011 Volume 028 Issue 02
The Cosmic Web! What Does Our Universe Look Like on the Largest Scale?
Astrophysics in 2006 3
Galaxy Data Name Constell
Arxiv:1007.2659V1 [Astro-Ph.SR] 15 Jul 2010 Aeteesasecletcrnmtr N Edsrb Why Describe Stars
MARGARET J. GELLER Education: University of California, Berkeley, BA
The Dark Matter Distribution in Abell 383: Evidence for a Shallow
The Universe Contents 3 HD 149026 B
Annual Report 2011
A Weak-Lensing Analysis of the Abell 383 Cluster ⋆
2016 Publication Year 2020-04-28T10:16:34Z Acceptance in OA@INAF the Galaxy Cluster Concentration-Mass Scaling Relation Title Gr
Dark Matter in Galaxy Clusters: Shape, Projection, and Environment
The Electromagnetic Radiation Field
The Galaxy Cluster Concentration-Mass Scaling Relation
Black Holes, Chaos in Universe, Processes in Space, Stars, Galaxies, Ordered Universe
Cluster Physics with Merging Galaxy Clusters
Resolving Sub-Kiloparsec Star-Forming Regions Within
Top View
Astronomy November
Dark Matter-3.Pdf
Appendix: Astronomical Distance and Energy Units
Bibliographie Complète
Intracluster Medium Entropy Profiles for a Chandra
Carnegie Mellon University MELLON COLLEGE of SCIENCE
ISSI Annual Report 2010/2011 Business Year 16
Sobre O Problema Da Materia Escura Fria Não Bariônica
Triaxiality, Principal Axis Orientation and Non-Thermal Pressure in Abell
A Redshift Survey of the Strong-Lensing Cluster Abell 383
Optical Emission Line Nebulae in Galaxy Cluster Cores 1
HST Senior Review Proposal 2013-2014 Annexes-A
2013.1 - Grade a & B Proposals
Scientia Volume 2 (2011)
Galaxies in Tonight's Lecture
Dark Matter in Galaxy Clusters: Shape, Projection, and Environment
Arxiv:1407.2260V4 [Astro-Ph.GA] 3 Nov 2014 Day Universe Are the first-Ranked Or Brightest Cluster Galaxies (BCG) in Rich Galaxy Clusters
Understanding the Role of the Environment in the Quenching of Galaxies)