Variation of Central Star Masses in Planetary Nebulae with Height above the Galactic Plane
There are various reasons for suspecting that the progenitor masses of planetarynebulae (PNe) decline with height z above the Galactic plane. This, if true,would also imply a similar decrease in mean central star masses <MCS>. We reporthere a further way in which such gradients may be determined. It...
保存先:
| 出版年: | Revista Mexicana de Astronomía y Astrofísica |
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| 第一著者: | |
| フォーマット: | Artigo |
| 言語: | Inglês |
| 出版事項: |
Universidad Nacional Autónoma de México
2004
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| 主題: | |
| オンライン･アクセス: | https://www.redalyc.org/articulo.oa?id=57140103 |
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