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Paper: The High Velocity Cloud HVC 487 and its Relationship to Magellanic Stream Gas
Volume: 166, Stromlo Workshop on High-Velocity Clouds
Page: 84
Authors: Sahu, Meena S.
Abstract: The line-of-sight to the H i-rich dwarf galaxy NGC 1705 intercepts the high velocity cloud HVC 487. The (Si/H) ratio (> 0.6(Si/H){_odot}) and low dust depletion derived for HVC 487 from archival GHRS data are consistent with an association with Magellanic Stream gas.
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