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Vol. 12 No. 1 (2002)
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Contributions
Vol. 12 No. 1 (2002)
Contributions
Implications of Dust for the Radiation Spectrum of Shell-Type PN Models
Kimeswenger S.
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Koller J.
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Kimeswenger S.
Institut für Astrophysik, Universität Innsbruck, Technikerstr. 25/8, A-6020 Innsbruck, Austria.
0000-0003-2379-0474
Koller J.
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PDF
PDF
Keywords
CIRCUMSTELLAR MATTER
LINE: PROFILES
BINARIES: SYMBIOTIC
PLANETARY NEBULAE: GENERAL
STARS: AGB AND POST-AGB
How to Cite
Implications of Dust for the Radiation Spectrum of Shell-Type PN Models. (2002).
Revista Mexicana De Astrofísica Y Astronomía Serie De Conferencias
,
12
(1), 164-164.
https://astronomia.unam.mx/journals/rmxac/article/view/2002rmxac..12..164k
hola
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Abstract
We have modeled the dust in extended PNe and found that the traditional methods used to derive dust temperature and dust-to-gas ratio from IRAS 25 and 60 mu m fluxes can be subject to large errors.
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