Lanean...
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...
Gorde:
| Argitaratua izan da: | Revista Mexicana de Astronomía y Astrofísica |
|---|---|
| Egile nagusia: | |
| Formatua: | Artigo |
| Hizkuntza: | Inglês |
| Argitaratua: |
Universidad Nacional Autónoma de México
2000
|
| Gaiak: | |
| Sarrera elektronikoa: | https://www.redalyc.org/articulo.oa?id=57100906 |
| Etiketak: |
Etiketa erantsi
Etiketarik gabe, Izan zaitez lehena erregistro honi etiketa jartzen!
|