Volume 401, Number 1, April I 2003
|Page(s)||205 - 214|
|Section||Interstellar and circumstellar matter|
|Published online||17 March 2003|
Kapteyn Astronomical Institute, PO Box 800, 9700 AV Groningen, the Netherlands
2 School of Science Education, ChungBuk National University, 48 Gaeshin-dong, CheongJu 361-763, South Korea
3 Dept. of Physics and Astronomy, Univ. of California, Los Angeles, CA 90095, USA
4 SRON National Institute for Space Research, PO Box 800, 9700 AV Groningen, the Netherlands
5 Laboratory for Astronomy and Solar Physics, Code 681, Goddard Space Flight Center, Greenbelt, MD 20771, USA
Corresponding author: S. R. Pottasch, firstname.lastname@example.org
Accepted: 15 January 2003
The ISO and IUE spectra of the “elliptical” nebula Hu 1-2 are presented. These spectra are combined with new, high resolution spectra in the visual wavelength region to obtain a complete, extinction corrected, spectrum. The chemical composition of the nebula is then calculated and compared to previous determinations. The abundances determined are the lowest yet found in the analysis of ISO data. The evolutionary significance is discussed.
Key words: ISM: abundances / planetary nebulae: individual: Hu 1-2 / infrared: ISM / ISM: lines and bands
© ESO, 2003
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