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"Superthin" spiral galaxies are so-called owing to their highly flattened, dynamically cold stellar disks and their lack of a visible spheroid component. These properties are evident because we are viewing these galaxies nearly exactly edge-on. The term "superthin" was coined by Jean Goad and Morton Roberts in their seminal 1981 paper, although Russian scientists had drawn attention to these intriguing "needle-like" galaxies in photographic sky surveys even earlier (e.g., Ogorodnikov 1958; Vorontsov-Vel'yaminov 1967). The structural simplicity and edge-on orientation of superthins makes these galaxies excellent laboratories for exploring how internal versus external processes regulate many of the key properties of disk galaxies, including their structures and star formation histories.
Available here are some data products from my own published studies of superthin galaxies. This compilation is a work in progress. Any use of these data should cite the reference(s) indicated. For additional data and information, see my complete list of publications.
Reference: Matthews &
Uson 2008a (AJ, 135, 291).
Reference: Matthews &
de Grijs 2004 (AJ, 128, 137).
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