Magellanov most
| Medzvezdni oblak | |
|---|---|
| Območje H I | |
| Opazovalni podatki: J2000.0 epoha | |
| Rektascenzija | 03h 11m |
| Deklinacija | -77.5° |
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 | uredi kodo]- ↑ 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)
