The Luminosity Function of PNe with different morphology

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dc.creatorMagrini, L.
dc.creatorCorradi, R. L. M.
dc.creatorLeisy, P.
dc.creatorScatarzi, A.
dc.creatorMorbidelli, L.
dc.creatorPerinotto, M.
dc.date2003-10-06
dc.date.accessioned2026-07-07T02:09:59Z
dc.date.available2026-07-07T02:09:59Z
dc.descriptionWe have analyzed the behaviour of various parameters of PNe in the Magellanic Clouds (MCs) and the Galaxy as a function of their morphology. The luminosity function of different morphological types has been built, finding that elliptical and round PNe dominate the bright cutoff both in the MCs and in the Galaxy. The dependence of the [OIII] absolute magnitude on chemical abundances has been investigated.
dc.description4 pages, 3 figures; to appear in ``Asymmetric Planetary Nebulae III'', ASP conf. series, in press (2003)
dc.identifierhttps://arxiv.org/abs/astro-ph/0310129
dc.identifierhttp://arxiv.org/abs/astro-ph/0310129
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6641
dc.subjectAstrophysics
dc.titleThe Luminosity Function of PNe with different morphology
dc.typetext

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