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NGC 1898
Remerciements – Unité 1
Yourthe Magazine for Alumni and Friends 2011 – 2012
Astro-Ph/9809362 28 Sep 1998 Subject Headings Subject Ofclusters
108 Afocal Procedure, 105 Age of Globular Clusters, 25, 28–29 O
Large Magellanic Cloud Star Clusters
Ngc Catalogue Ngc Catalogue
Continuum Theory: Physical Nature Copyright © 2010 Miles F Osmaston Viewed from a Deeper Level; a Rewarding Replacement for SR/GR
Abundances in Large Magellanic Cloud Star Clusters
Continuum Theory: Physical Nature Viewed from a Deeper Level; a Rewarding Replacement for SR/GR and Its Mortal Inconsistencies*
The Galaxies of the Local Group Sidney Van Den Bergh Index More Information
IAU Xxiind General Assembly -The Hague 1994 Editor: SETH SHOSTAK Associate Editor: RENÉ GENEE No
Stars, Galaxies, and Beyond, 2012
Arxiv:0705.3464V1
Washington Photometry of Five Star Clusters in the Large Magellanic
Download This Article in PDF Format
Searching for Chemical Inhomogeneities in Open Clusters Analysis of the CN and CH Molecular Band Strengths in NGC 2158, NGC 2420, NGC 2682, NGC 7789, and Berkeley 29
A DATABASE of 2MASS NEAR-INFRARED COLORS of MAGELLANIC CLOUD STAR CLUSTERS Peter M
Old and Intermediate-Age Stellar Populations in the Magellanic Clouds
Top View
HST Colour–Magnitude Diagrams of Six Old Globular Clusters in the LMC
Wolf-Rayet Stars: Extremely Hot, Luminous and Massive
The WAGGS Project-I. the Wifes Atlas of Galactic Globular Cluster Spectra
THE MAGELLANIC CLOUDS NEWSLETTER an Electronic Publication Dedicated to the Magellanic Clouds, and Astrophysical Phenomena Therein
1982Apj. . .261. . .85R the Astrophysical Journal, 261:85-101, 1982 October 1 © 1982. the American Astronomical Society. All Ri
Role of Host Galaxy in the Formation of Multiple Stellar Populations: Analysis of NGC 1786 and NGC 1898
Arxiv:Astro-Ph/0512132V1 5 Dec 2005
Two Kinematically Distinct Old Globular Cluster Populations in the Large Magellanic Cloud
ASTRONOMY and ASTROPHYSICS Age and Metallicity for Six LMC