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- W2015743537 abstract "We have conducted a deep search for neutral hydrogen gas associated with the faint optical jets of NGC 1097 using the Very Large Array. Measurable H I would have been expected if the jets were tidal in origin given their moderately blue optical and near-infrared colors. The jets are free of H I emission to a limiting surface density (Σ) of 0.06 M☉ pc-2 (3 σ) over a 1102 km s-1 velocity range. We also rule out extended H I emission down to 0.02 M☉ pc-2 (3 σ, ΔV = 45 km s-1) within a 4' FWHM aperture centered on the right-angle turn in jet R1. We have detected an H I source [M = (5.1 ± 1.0) × 106 M☉] coincident with a small edge-on spiral or irregular galaxy (NGC 1097B) 12' southwest of NGC 1097, situated between two jets. Two other ~106 M☉ H I point sources in the field are considered marginal detections. Neither are associated with the optical jets." @default.
- W2015743537 created "2016-06-24" @default.
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- W2015743537 date "2003-03-01" @default.
- W2015743537 modified "2023-09-26" @default.
- W2015743537 title "A Minor‐Merger Interpretation for NGC 1097’s “Jets”" @default.
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- W2015743537 doi "https://doi.org/10.1086/345978" @default.
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