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The Frequency of Barred Spiral Galaxies in the Near-Infrared*
We have determined the fraction of barred galaxies in the H-band for a statistically well-defined sample of 186 spirals drawn from the Ohio State University Bright Spiral Galaxy Survey. We find 56%Expand
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A Multivariate Statistical Analysis of Spiral Galaxy Luminosities. I. Data and Results
We have performed a multiparametric analysis of luminosity data for a sample of 234 normal spiral and irregular galaxies observed in X-rays with the Einstein Observatory. This sample isExpand
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Near-Infrared and Optical Morphology of Spiral Galaxies
We announce the initial release of data from the Ohio State University (OSU) Bright Spiral Galaxy Survey, a BVRJHK imaging survey of a well-defined sample of 205 bright, nearby spiral galaxies. WeExpand
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A COSMOS study of the structure and content of NGC 6822
A COSMOS survey of deep Schmidt plates in four colors is used to examine the distribution of stars and unresolved light in the local group dwarf irregular galaxy NGC 6822. Global color-magnitudeExpand
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The Visibility of Galactic Bars and Spiral Structure at High Redshifts
We investigate the visibility of galactic bars and spiral structure in the distant universe by artificially redshifting 101 B-band CCD images of local spiral galaxies from the Ohio State UniversityExpand
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Morphological classification of the OSU Bright Spiral Galaxy Survey
To quantify the distribution of bar shapes in spiral galaxies, we have analysed 113 H-band and 89 B-band galaxy images from the Ohio State University Bright Spiral Galaxy Survey. Parameters measuringExpand
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A multiparametric analysis of the Einstein sample of early-type galaxies. 1: Luminosity and ISM parameters
We have conducted bivariate and multivariate statistical analysis of data measuring the luminosity and interstellar medium of the Einstein sample of early-type galaxies (presented by Fabbiano, Kim, &Expand
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The structure of the sculptor dwarf elliptical galaxy. I - The radial profile
Automated star counts of the UK Schmidt telescope unit have been used to obtain the radial profile of the Sculptor dwarf elliptical galaxy. Adopting a core radius of 8.9 arcmin and a tidal radius ofExpand
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Star formation in the disks of H I-rich S0 galaxies
We present the results of a H-alpha emission-line imaging survey of a sample of neutral-gas-rich S galaxies. We find evidence of disk H II regions in 14 of our sample of 32 galaxies, detect nuclearExpand
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A Cosmos study of IC 1613
A Cosmos survey of deep Schmidt plates in three colors is used to examine the distribution of stars and unresolved light in the Local Group dwarf irregular galaxy IC 1613. Color-magnitude diagramsExpand
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