Magellanic clouds planetary nebulae: an updated view on stellar evolution and populations
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| Format: | Artículo científico |
| Language: | en |
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Universidad Nacional Autónoma de México
2002
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| _version_ | 1876429819546173440 |
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| author | L. Stanghellini |
| author_facet | L. Stanghellini |
| contents | Magellanic clouds planetary nebulae: an updated view on stellar evolution and populations L. Stanghellini R. A. Shaw M. Mutchler Física, Astronomía y Matemáticas TION STARS: EVOLU MAGELLANIC CLOUDS PLANETARY NEBULAE: GENERAL Planetary Nebulae (PNe) in the Magellanic Clouds are studied to understand stellar populations and evolutionof low- and intermediate-mass stars in di erent chemical environments. Using HST observations from ourLMC and SMC PN morphological survey and from the HST Data Archive, we look at the relations betweenPN morphology and their evolution and populations. In this paper we show some of our recent results on theserelations, in an historical context. 2002 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57112038 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.12 |
| format | Artículo científico |
| id | redalyc_57112038 |
| institution | Redalyc |
| language | en |
| publishDate | 2002 |
| publisher | Universidad Nacional Autónoma de México |
| spellingShingle | Magellanic clouds planetary nebulae: an updated view on stellar evolution and populations L. Stanghellini Física, Astronomía y Matemáticas TION STARS: EVOLU MAGELLANIC CLOUDS PLANETARY NEBULAE: GENERAL Magellanic clouds planetary nebulae: an updated view on stellar evolution and populations L. Stanghellini R. A. Shaw M. Mutchler Física, Astronomía y Matemáticas TION STARS: EVOLU MAGELLANIC CLOUDS PLANETARY NEBULAE: GENERAL Planetary Nebulae (PNe) in the Magellanic Clouds are studied to understand stellar populations and evolutionof low- and intermediate-mass stars in di erent chemical environments. Using HST observations from ourLMC and SMC PN morphological survey and from the HST Data Archive, we look at the relations betweenPN morphology and their evolution and populations. In this paper we show some of our recent results on theserelations, in an historical context. 2002 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57112038 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.12 |
| title | Magellanic clouds planetary nebulae: an updated view on stellar evolution and populations |
| topic | Física, Astronomía y Matemáticas TION STARS: EVOLU MAGELLANIC CLOUDS PLANETARY NEBULAE: GENERAL |
| url | https://www.redalyc.org/articulo.oa?id=57112038 |