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Donovan L. Domingue

Researcher at Georgia College & State University

Publications -  22
Citations -  412

Donovan L. Domingue is an academic researcher from Georgia College & State University. The author has contributed to research in topics: Galaxy & Spiral galaxy. The author has an hindex of 12, co-authored 20 publications receiving 369 citations. Previous affiliations of Donovan L. Domingue include Association of Universities for Research in Astronomy & University of Alabama.

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Journal ArticleDOI

Local benchmarks for the evolution of major-merger galaxies—spitzer observations of a k-band selected sample

C. Kevin Xu, +11 more
- 10 Apr 2010 - 
TL;DR: In this article, the authors present Spitzer observations for a sample of close major-merger galaxy pairs (KPAIR sample) selected from cross-matches between the Two Micron All Sky Survey and Sloan Digital Sky Survey Data Release 3.
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Seeing Galaxies through Thick and Thin. II. Direct Measures of Extinction in Spiral Disks through Spectroscopy of Overlapping Galaxies

Donovan L. Domingue, +4 more
- 10 Dec 2000 - 
TL;DR: In this article, the authors used slit spectroscopy of overlapping pairs of galaxies to directly determine the extinction in disks of foreground spiral galaxies, where the Doppler shifts of pair members were determined via cross-correlation, and their relative correlation amplitudes were used to separate their contributions to the combined spectra in regions of overlap.
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Mapping IR Enhancements in Closely Interacting Spiral-Spiral Pairs: I. ISO CAM and ISO SWS Observations

Cong Xu, +6 more
- 01 Jan 2000 - 
TL;DR: In this article, the authors used mid-infrared (MIR) imaging and spectroscopic observations for a well-defined sample of eight closely interacting (CLO) pairs of spiral galaxies that have overlapping disks and show enhanced far infrared (FIR) emission.
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2MASS/SDSS Close Major-Merger Galaxy Pairs

Donovan L. Domingue, +5 more
- 20 Apr 2009 - 
TL;DR: In this paper, the authors select a close "major-merger candidate" galaxy pair sample in order to calculate the K_s luminosity function and pair fraction representative of the merger/interaction component of galaxy evolution in the local universe.
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Dust in Spiral Galaxies: Comparing Emission and Absorption to Constrain Small-Scale and Very Cold Structures*

Donovan L. Domingue, +6 more
- 01 Oct 1999 - 
TL;DR: In this article, the authors compare column densities and dust masses derived from the absorption and emission techniques using the galaxy-overlap technique in the optical, with measures of the dust grains' thermal emission from 50-2000 μm, using ISOPHOT on board Infrared Space Observatory (ISO) and SCUBA at the James Clerk Maxwell Telescope.