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Dorado Group
Arxiv:2009.04090V2 [Astro-Ph.GA] 14 Sep 2020
A Comprehensive Comparative Test of Seven Widely Used Spectral Synthesis Models Against Multi-Band Photometry of Young Massive-Star Clusters
Dorado and Its Member Galaxies II: a UVIT Picture of the NGC 1533 Substructure
Jan / Feb 2015 1
Galactic Recycling: the Hi Ring Around Ngc 1533
2019 Publication Year 2020-11-30T11:15:22Z Acceptance
1. INTRODUCTION Dwarf Galaxies Are the Most Common Type of Galaxies in Ferguson 1989; Bothun, Impey, & Malin 1991; Groups: the Local Universe
Arxiv:2011.03324V2 [Astro-Ph.GA] 9 Nov 2020 Hc Soeae Yar,Ic Ne Otatn.NAS5–2655 No
Revista Astronômica
Observer's Guide to Galaxies
The Universe Contents 3 HD 149026 B
How Astronomical Objects Are Named
Dorado and Its Member Galaxies II. a UVIT Picture of the NGC 1533 Substructure
Katherine Elizabeth Hollyhead Liverpool John Moores University
A Misty Cloud on Our Doorstep
A Deep Look at NGC1533 in the Dorado Group with VST
Properties of the Cluster Population of NGC 1566 and Their Implications
THE MAGELLANIC CLOUDS NEWSLETTER an Electronic Publication Dedicated to the Magellanic Clouds, and Astrophysical Phenomena Therein
Top View
Search for Star Cluster Age Gradients Across Spiral Arms of Three LEGUS Disc Galaxies
Claudia Mendes De Oliveira on Behalf of the S-PLUS Collaboration La Plata, Febr Ar 16, 2020 Photometry Spectroscopy Vs
Kinematics, Substructure and Luminosity-Weighted Dynamics of Six Nearby Galaxy Groups
The Dependence of the Hierarchical Distribution of Star Clusters on Galactic Environment
Search for the Brightest Stars in Galaxies Outside the Local Group ∗
Grand Swirls from Hubble 12 June 2014
A Comprehensive Comparative Test of Seven Widely Used Spectral Synthesis Models Against Multi-Band Photometry of Young Massive-Star Clusters
Designed by Marc Rouault in 2020 Available in 294 Styles Licenses for Web, Desktop, & App 1 Roman Width / Weight Overview
LEXSEE 43 UCLA L. REV. 839 Copyright (C) the Regents of The