Volume 486, Number 1, July IV 2008
|Page(s)||221 - 228|
|Section||Interstellar and circumstellar matter|
|Published online||15 May 2008|
Emission line profiles as a probe of physical conditions in planetary nebulae
Department of Physics, University of Hong Kong, Hong Kong e-mail: email@example.com
Accepted: 9 April 2008
Aims. We present an analysis of physical conditions in planetary nebulae (PNe) in terms of collisionally-excited line (CEL) and optical-recombination line (ORL) profiles. We aim to investigate whether line profiles could be used to study the long-standing CEL/ORL abundance-discrepancy problem in nebular astrophysics.
Methods. Using 1D photoionization models and their assumed velocity fields, we simulate the line profiles of various ionic species. We attempt to use our model to account for the observed CEL and ORL profiles. As a case study we present a detailed study of line profiles of the low-excitation planetary nebula (PN) IC 418.
Results. Our results show that the profiles of classical temperature and density diagnostic lines, such as [O iii] 4363, 5007, [S ii] 6716, 6731, and [Ar iv] 4711, 4740, provide a powerful tool to study nebular temperature and density variations. The method enables the CEL/ORL abundance-discrepancy problem to be studied more rigorously than before. A pure photoionization model of a chemically-homogeneous nebula seems to explain the observed disagreements in the profiles for the [O iii] λ4363 and the λ5007 lines, but cannot account for the differences between the [O iii] CELs and the O ii ORLs. We also investigate the temperature and density variations in the velocity space of a sample of PNe, which are found to be insignificant.
Key words: ISM: planetary nebulae: general / line: profiles
© ESO, 2008
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.