Volume 421, Number 3, July III 2004
|Page(s)||1051 - 1061|
|Section||Interstellar and circumstellar matter|
|Published online||29 June 2004|
Indian Institute of Astrophysics, Koramangala II Block, Bangalore – 560034, India
2 Kapteyn Astronomical Institute, PO Box 800, 9700 AV Groningen, The Netherlands
3 ISO Data Centre, Science Operations and Data Systems Division, Research and Scientific Support Department of ESA, Villafranca del Castillo, Apartado de Correos 50727, 28080 Madrid, Spain
Corresponding author: R. Surendiranath, firstname.lastname@example.org
Accepted: 16 March 2004
ISO and IUE spectra of the round planetary nebula Me 2-1 are combined with visual spectra taken from the literature to obtain for the first time a complete extinction-corrected spectrum. With this, the physico-chemical characteristics of the nebula and its central star are determined by various methods including photoionization modeling using Cloudy. The results of the modeling are compared to those derived from a more classical, simple abundance determination approach. A discussion is presented on the validity of the different methods used and assumptions made. Finally, the main results are interpreted in terms of the evolutionary stage of Me 2-1 and its central star.
Key words: ISM: abundances / planetary nebulae: individual: Me 2-1 / infrared: ISM / ISM: lines and bands
Based on observations with ISO, an ESA project with instruments funded by ESA Member States (especially the PI countries: France, Germany, The Netherlands and the UK) and with the participation of ISAS and NASA. This research has also used archival IUE and HST data.
© ESO, 2004
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