Mark Hancock
East Tennessee State University
18 Papers
17 Citations
Mark Hancock is an academic researcher from East Tennessee State University. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 7, co-authored 18 publications. Previous affiliations of Mark Hancock include University of California, Riverside.
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Papers
Candidate Tidal Dwarf Galaxies in Arp 305: Lessons on Dwarf Detachment and Globular Cluster Formation
TL;DR: In this paper, a large UV imaging survey of interacting galaxies selected from the Arp (1996) Atlas using the GALEX telescope was conducted to search for Tidal Dwarf Galaxies and to study star formation in tidal features.
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Star Formation and the Interstellar Medium in Nearby Tidal Streams (SAINTS)
TL;DR: In this paper, the authors compare Spitzer Infrared Spectrograph observations of SQ-A and SQ-B in Stephan's Quintet, Ambartzumian's knot in Arp 105, Arp 242-N3, and Arp 87-N1, a bridge star forming region.
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Tidal Dwarf Galaxies, Accretion Tails, and `Beads on a String' in the `Spirals, Bridges, and Tails' Interacting Galaxy Survey
TL;DR: The authors used the GALEX ultraviolet telescope to study stellar populations and star formation morphology in a well-defined sample of more than three dozen nearby optically-selected pre-merger interacting galaxy pairs.
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Spirals, Bridges, and Tails: A GALEX UV Atlas of Interacting Galaxies
TL;DR: In this article, the authors used the GALEX ultraviolet telescope to study stellar populations and star formation morphology in a well-defined sample of 42 nearby optically-selected pre-merger interacting galaxy pairs.
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Large-scale Star Formation Triggering in the Low-mass Arp 82 System: A Nearby Example of Galaxy Downsizing Based on UV/Optical/Mid-IR Imaging
Mark Hancock,Beverly J. Smith,Curtis Struck,Mark L. Giroux,Philip N. Appleton,Vassilis Charmandaris,Vassilis Charmandaris,William T. Reach +7 more
TL;DR: In this article, the authors investigate the multiwavelength properties of several individual star forming complexes (clumps) using optical and UV colors, EW(Halpha), and population synthesis models.