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HST detection of spiral structure in two Coma Cluster dwarf galaxies

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arxiv astro-ph/0308241 v1 pith:MXLP25LY submitted 2003-08-14 astro-ph

HST detection of spiral structure in two Coma Cluster dwarf galaxies

classification astro-ph
keywords clusterdwarfgalaxiescomagalaxyspiralspiral-likestructure
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We report the discovery of (stellar) spiral-like structure in Hubble Space Telescope images of two dwarf galaxies (GMP 3292 and GMP 3629) belonging to the Coma cluster. GMP 3629 is the faintest such galaxy detected in a cluster environment, and it is the first such galaxy observed in the dense Coma cluster. The large bulge and the faintness of the broad spiral-like pattern in GMP 3629 suggests that its disk may have been largely depleted. >We may therefore have found an example of the ``missing link'' in theories of galaxy evolution which have predicted that dwarf spiral galaxies, particularly in clusters, evolve into dwarf elliptical galaxies.

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