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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Outside-in Shrinking of the Star-forming Disk of Dwarf Irregular Galaxies
TL;DR: In this paper, the authors studied multi-band surface brightness profiles of a representative sample of 34 nearby dwarf irregular galaxies and derived the stellar mass surface density distributions and the star formation rate averaged over three different timescales: recent 0.1 Gyr, 1 Gyr and a Hubble time.
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The K Band Luminosity Function in Galaxy Clusters to z ~ 1
TL;DR: In this article, the authors present a K-band luminosity function for galaxies in a heterogeneous sample of 38 clusters at 0.1 0.7 (0) in the universe.
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Star Formation in the Field and Clusters of NGC 5253
Christy A. Tremonti,Christy A. Tremonti,Daniela Calzetti,Claus Leitherer,Timothy M. Heckman,Timothy M. Heckman +5 more
TL;DR: In this paper, the star formation history of both the bright star clusters and the diffuse field star population in the dwarf starburst galaxy NGC 5253 was investigated using long-slit ultraviolet spectroscopy obtained with the Space Telescope Imaging Spectrograph.
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The Distance to the M31 Globular Cluster System
TL;DR: The distance to the centroid of the M31 globular cluster system was determined by fitting theoretical isochrones to the observed red giant branches of 14 globular clusters in M31 as discussed by the authors.
Journal ArticleDOI
Deep ACS Imaging of the Halo of NGC 5128: Reaching the Horizontal Branch*
Marina Rejkuba,Laura Greggio,William E. Harris,Gretchen L. H. Harris,Eric W. Peng,Eric W. Peng +5 more
TL;DR: Using the Hubble Space Telescope (HST) Wide Field Camera (WFC) of the Advanced Camera for Surveys (ACS), the authors obtained deep (V, I) photometry of an outer halo field in NGC 5128, to a limiting magnitude of I 29.