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- W2758559780 abstract "We present H i synthesis imaging of the giant elliptical galaxy IC 1459 and its surroundings with the Australia Telescope Compact Array. Our search for extended H i emission revealed a large complex of H i clouds near IC 1459, likely to be the debris from tidal interactions with neighbouring galaxies. The total H i mass (∼109 M⊙) in the detected clouds spans 250 kpc from the north-east of the gas-rich spiral NGC 7418A to the south-east of IC 1459. The extent and mass of the H i debris, which shows rather irregular morphology and kinematics, are similar to those in other nearby groups. Together with H i clouds recently detected near two other IC 1459 group members, namely IC 5270 and NGC 7418, using phased-array feeds on the Australian Square Kilometre Array Pathfinder, the detected debris make up a significant fraction of the group's intergalactic medium." @default.
- W2758559780 created "2017-10-06" @default.
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- W2758559780 date "2017-09-26" @default.
- W2758559780 modified "2023-10-06" @default.
- W2758559780 title "H i debris in the IC 1459 galaxy group" @default.
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- W2758559780 doi "https://doi.org/10.1093/mnras/stx2475" @default.
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