Magellanov most

Magellanov most
Medzvezdni oblak
Območje H I
Opazovalni podatki: J2000.0 epoha
Rektascenzija	03h 11m
Deklinacija	-77.5°
	Glej tudi: seznami meglic

Magellanov most je tok nevtralnega vodika, ki povezuje Veliki in Mali Magellanov oblak.^[1] Večinoma ga sestavlja plin z nizko vsebnostjo težjih elementov, vendar je bilo v njem najdenih nekaj zvezd.^[2]^[3]

Sklici uredi

↑ 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) Ameriško astronomsko društvo, (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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[putn-1] 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-2] Lehner, Nicolas. "FUSE Observations of the Magellanic Bridge." (Abstract) Ameriško astronomsko društvo, (199th AAS Meeting, #65.06); Bulletin of the American Astronomical Society, Vol. 33, p.1408.

[3] 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)

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