Journal ArticleDOI
Reddenings derived from H I and galaxy counts : accuracy and maps.
D. Burstein,C. Heiles +1 more
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This article is published in The Astronomical Journal.The article was published on 1982-08-01. It has received 1025 citations till now. The article focuses on the topics: Disc galaxy & Interacting galaxy.read more
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Journal ArticleDOI
Analysis of UBV photometry in selected area 133
TL;DR: In this paper, the authors interpret the de-reddened UBV data for the field SA 133 to deduce the stellar density and metallicity distribution functions, and the agreement of the luminosity function for dwarfs and sub-giants with the one of Hipparcos confirms the empirical method used for their separation.
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Determination of Reddening and Age for Ten Large Magellanic Cloud Star Clusters from Integrated Spectroscopy
Andrea Veronica Ahumada,Andrea Veronica Ahumada,Luis R. Vega,Luis R. Vega,Juan J. Clariá,Juan J. Clariá,M. A. Oddone,Tali Palma,Tali Palma,Tali Palma +9 more
TL;DR: In this article, the authors presented flux-calibrated integrated spectra in the optical range (3700-6800 A) obtained at Complejo Astronomico El Leoncito (CASLEO, Argentina) for a sample of 10 concentrated star clusters belonging to the Large Magellanic Cloud (LMC).
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Optical observations of a newly identified compact galaxy group near the Zone of Avoidance
S. Temporin,Stefano Ciroi +1 more
TL;DR: In this paper, a new group of galaxies, CG J0247+44.9, was identified, consisting of six members, two of which are in close interaction (IRAS 02443+4437), which satisfies Hickson's criteria (Hickson 1997 for Compact Groups (CGs)).
Journal ArticleDOI
The Stellar Populations of M32: Resolving the nearest elliptical with HST ACS/HRC
Antonela Monachesi,Scott Trager,Tod R. Lauer,Wendy L. Freedman,Alan Dressler,Carl J. Grillmair,Kenneth J. Mighell +6 more
TL;DR: In this paper, the authors presented the deepest color-magnitude diagram (CMD) of M32 to date, obtained from deep (F435W, F555W) photometry of HST ACS/HRC images.
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Reddening free distance determination via Cepheid variables
TL;DR: In this article, a long-term project initiated four years ago with the aim of establishing a consistent set of distances founded on ground-based photometry of Cepheid variables in the nearest late-type galaxies in the Local Group, or just beyond it is reported on.