FCC 35 and Its H I Companion: Multiwavelength Observations and Interpretation

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© 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation M. E. Putman et al 1998 AJ 115 2345 DOI 10.1086/300367

1538-3881/115/6/2345

Abstract

     The Fornax Cluster galaxy FCC 35 shows an unusual multiply peaked integrated H I profile. We have now observed FCC 35 with the Australia Telescope Compact Array and have found a compact H I source with MHI = 2.2 × 108 M and a spatially overlapping complex of H I gas with the same mass. By combining optical observations with the H I data, we are able to identify FCC 35 as a young compact source of star formation with a nearby intergalactic H I cloud that is devoid of stars. We classify FCC 35 as a blue compact dwarf or H II galaxy, having large amounts of neutral hydrogen, very blue colors (U - V = 0.1), and a low-metallicity spectrum with strong narrow emission lines. Together with the presence of the H I cloud, this suggests that FCC 35 is the result of a recent interaction within the Fornax Cluster.

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10.1086/300367