Physical conditions derived from O II recombination lines in planetary nebulae and their implications

Peimbert, A.; Peimbert, M.; Delgado-Inglada, G.; García-Rojas, J.; Peña, M.
Bibliographical reference

Revista Mexicana de Astronomía y Astrofísica Vol. 50, pp. 329-340 (2014)

Advertised on:
10
2014
Number of authors
5
IAC number of authors
1
Citations
19
Refereed citations
13
Description
Based on high quality observations of multiplet V1 of O II and the NLTE atomic computations for O II we study the density and temperature of a sample of PNe. We find that, in general, the densities derived from recombination lines of O II are similar to the densities derived from forbidden lines. This implies that the signature for oxygen rich clumps of high density and low temperature is absent in most of the objects of our sample. Electron pressures derived from the hotter zones are similar or slightly larger than those derived from the colder zones, suggesting the presence of shock waves. The average temperatures and t^{2} values derived from H, He and O lines are similar and consistent with chemical homogeneity. These results suggest that the abundances of these objects are the ones derived from recombination lines.
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Physics of Ionized Nebulae

The research that is being carried out by the group can be condensed into two main lines: 1) Study of the structure, dynamics, physical conditions and chemical evolution of Galactic and extragalactic ionized nebulae through detailed analysis and modelization of their spectra. Investigation of chemical composition gradients along the disk of our

Jorge
García Rojas