WHAT CAN WE LEARN ABOUT THE KINEMATICS OF BRIGHT EXTRAGALACTIC PLANETARY NEBULAE?
We present high resolution spectroscopy in the [O III]-5007 and H lines of bright planetary nebulae in the Milky Way bulge and the dwarf galaxies M32, Fornax, Sagittarius, and NGC 6822 obtained at the Observatorio Astronómico Nacional in the Sierra San Pedro Mártir using the Manchester Echelle Spec...
Tallennettuna:
| Julkaisussa: | Revista Mexicana de Astronomía y Astrofísica |
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| Päätekijät: | , , , , |
| Aineistotyyppi: | Artigo |
| Kieli: | Inglês |
| Julkaistu: |
Universidad Nacional Autónoma de México
2009
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| Aiheet: | |
| Linkit: | https://www.redalyc.org/articulo.oa?id=57112175012 |
| Tagit: |
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