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NGC 1987
Expected Differences Between AGB Stars in the LMC and the SMC Due to Differences in Chemical Composition
Controversial Age Spreads from the Main Sequence Turn-Off and Red Clump in Intermediate-Age Clusters in the LMC ? F
Population Parameters of Intermediate-Age Star Clusters in the Large Magellanic Cloud
Ngc Catalogue Ngc Catalogue
Chemical Evolution of the Large Magellanic Cloud)
Coin Auction Saturday, August 25Th, 2018 10 AM FHTC: 3301 W
A Catalogue of Integrated H-Alpha Fluxes for 1258 Galactic Planetary Nebulae
INFRARED SURFACE BRIGHTNESS FLUCTUATIONS of MAGELLANIC STAR CLUSTERS1 Rosa A
Star Formation and Molecular Clouds Towards the Galactic Anti-Center
Galactic Hα Emission Line Studies Using DEFPOS at the T¨UB˙ITAK
Star Forming Regions in Cepheus
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
1983Apj. . .266. .105P the Astrophysical Journal, 266:105-129, 1983 March 1 © 1983. the American Astronomical Society. All Righ
Controversial Age Spreads from the Main Sequence Turn-Off and Red Clump in Intermediate-Age Clusters in the LMC?
Globular Clusters As Probes of Galaxy Formation
1982Apj. . .261. . .85R the Astrophysical Journal, 261:85-101, 1982 October 1 © 1982. the American Astronomical Society. All Ri
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Integratedlight VRI Imaging Photometry of Globular Clusters In
An X-Ray Study of Massive Star Forming Regions With
SAO-6M Telescope Spectroscopic Observations of Globular Clusters in Nearby Galaxies
Multiple Stellar Populations in Magellanic Clouds Clusters
Astro-Ph/9409084 29 Sep 94 B Oni 33 Erraro Atorio Astronomico Y Usi P
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AL 37907:: a a Fax: 39-51-259407 F
Arxiv:1105.1317V2 [Astro-Ph.SR] 16 May 2011 U Hlegsoe H Atdcd.I Snwkonta the That Known As Seri- Such Now Galaxy Faced Is Our Has It in Gcs Scenario Decade