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Title:
Resolved Galaxies in the Spitzer Survey of the Taurus Molecular Cloud
Authors:
Spuck, Timothy; Rebull, L.; McCabe, C.; Noriega-Crespo, A.; Carey, S.; Brooke, T.; Huard, T.; Fukagawa, M.; Hines, D.; Padgett, D.; Terebey, S.; Stapelfeldt, K.; Hicks, K.; Holcomb, A.; McClintock, C.; McCool, A.; Morton, P.
Affiliation:
AA(Oil City High School/Spitzer), AB(Spitzer Science Center), AC(Spitzer Science Center), AD(Spitzer Science Center), AE(Spitzer Science Center), AF(Spitzer Science Center), AG(Spitzer Science Center), AH(Nagoya University, Japan), AI(Space Science Institute), AJ(Spitzer Science Center), AK(CSULA), AL(JPL), AM(Oil City High School/Spitzer), AN(Oil City High School/Spitzer), AO(Oil City High School/Spitzer), AP(Oil City High School/Spitzer), AQ(Oil City High School/Spitzer)
Publication:
American Astronomical Society, AAS Meeting #211, #12.18; Bulletin of the American Astronomical Society, Vol. 39, p.753
Publication Date:
12/2007
Origin:
AAS
Bibliographic Code:
2007AAS...211.1218S

Abstract

In the 44-square-degree Spitzer map of the main Taurus cloud obtained using the IRAC and MIPS cameras on the Spitzer Space Telescope, many resolved galaxies can be found. Simply locating this population is important, at the very least to distinguish candidate Taurus association members from resolved galaxies. We have identified the resolved galaxy population. We present multi-color thumbnail images of typical galaxies, and place them into the Hubble Sequence where possible.
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