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- W2019245087 abstract "The H i and optical properties of the NGC 428 galaxy field are presented. Three galaxies in this system are found to contain H i. The largest of these is NGC 428 which has undergone strong recent star formation in its spiral arms where the H i surface density exceeds ≈ 8 × 1020 cm−2. To the north of NGC 428 there is a low surface brightness galaxy (0110+008) with μ 0B=25.0 mag arcsec−2 and with a peak H i column density of ∼ 2 × 1020 cm−2. Additionally there is an H i tail lying to the south of NGC 428 with a peak H i column density of ∼ 1 × 1020 cm− which is connected to NGC 428 and extends to ∼ 2.5 Holmberg radii. This tail has no associated optical emission to ∼ 27 μb mag arcsec−2. It is postulated that the low H i surface density of the tail has inhibited star formation. Possible formation scenarios for the H i tail and low surface brightness galaxy 0110+008 are discussed." @default.
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- W2019245087 date "1996-07-11" @default.
- W2019245087 modified "2023-10-05" @default.
- W2019245087 title "H I and optical observations of the NGC 428 field" @default.
- W2019245087 doi "https://doi.org/10.1093/mnras/281.2.393" @default.
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