|H I region|
|Observation data: J2000.0 epoch|
|Right ascension||03h 11m|
|See also: Lists of nebulae|
The Magellanic Bridge is a stream of neutral hydrogen that links the two Magellanic Clouds. It is mostly a low-metallicity gas feature, though a few stars have been found inside it. It should not be confused with the Magellanic Stream, which links the Magellanic Clouds to the Milky Way. It was discovered in 1963 by J. V. Hindman et al.
- Putman, M. E. (2013). "The Magellanic System's Interactive Formations" (Free PDF download). Publications of the Astronomical Society of Australia 17: 1. Bibcode:2000PASA...17....1P. doi:10.1071/AS00001.
- Lehner, Nicolas. "FUSE Observations of the Magellanic Bridge." (Abstract) American Astronomical Society, (199th AAS Meeting, #65.06); Bulletin of the American Astronomical Society, Vol. 33, p.1408.
- Lehner, NNicolas "FUSE Observations of the Magellanic Bridge Gas toward Two Early-Type Stars: Molecules, Physical Conditions, and Relative Abundance." arXiv preprint astro-ph/0206250 (2002)
- SIMBAD, "Magellanic Bridge" (accessed 12 April 2010)
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