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Hot gas and the gaseous structure of the galaxy
Major advances have been made in the past decade in our knowledge of the hotinterstellar gas of our Milky Way galaxy. The Di use X-ray Spectrometer obtainedspectra in the 0.15{0.28 keV range from the Galactic plane (i.e., from the LocalBubble) that show emission lines and blends. These spectra conrm...
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| Pubblicato in: | Revista Mexicana de Astronomía y Astrofísica |
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| Autore principale: | |
| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
Universidad Nacional Autónoma de México
2000
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| Soggetti: | |
| Accesso online: | https://www.redalyc.org/articulo.oa?id=57100906 |
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