A new determination of the rotation curve from galactic disk planetary nebulae
The galactic rotation curve is determined on the basis of a large sample ofplanetary nebulae with known radial velocities. Four distance scales are adoptedand the curve is established for galactocentric distances of 4 to 14 kpc, approximately,adopting R0 = 8:5 kpc for the galactocentric distance of...
保存先:
| 出版年: | Revista Mexicana de Astronomía y Astrofísica |
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| 主要な著者: | , |
| フォーマット: | Artigo |
| 言語: | Inglês |
| 出版事項: |
Universidad Nacional Autónoma de México
2005
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| 主題: | |
| オンライン･アクセス: | https://www.redalyc.org/articulo.oa?id=57141202 |
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