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A&A 393, 285-294 (2002)
DOI: 10.1051/0004-6361:20020986
Abundances of Planetary Nebula NGC 5315
S. R. Pottasch1, D. A. Beintema1, 2, J. Bernard Salas1, 2, J. Koornneef3 and W. A. Feibelman41 Kapteyn Astronomical Institute, PO Box 800, 9700 AV Groningen, The Netherlands
2 SRON National Institute for Space Research, PO Box 800, 9700 AV Groningen, The Netherlands
3 Infostrait bv, Postbus 901, 7301 BD Apeldoorn, The Netherlands
4 Laboratory for Astronomy and Solar Physics, Code 681, Goddard Space Flight Center, MD, USA
(Received 13 May 2002 / Accepted 1 July 2002 )
Abstract
The ISO and IUE spectra of the elliptical nebula
NGC 5315
is presented. These spectra are combined with the spectra in the visual
wavelength region to obtain a complete, extinction corrected, spectrum. The
chemical composition of the nebulae is then calculated and compared to
previous determinations. The HST NICMOS observations of the nebula in 3 emission lines are also presented. These observations
are used to determine
the helium abundance as a function of position in the nebula. A discussion
is given of possible evolutionary effects.
Key words: ISM: abundances -- planetary nebulae: individual: NGC 5315 -- infrared: ISM -- ISM: lines and bands
Offprint request: S. R. Pottasch, pottasch@astro.rug.nl
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© ESO 2002
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