Spectroscopic observations of the planetary nebula ME 2-1

Details Spectroscopic observations of the planetary nebula ME 2-1 Spectroscopic observations of the planetary nebula ME 2-1

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994pasp..106..619m&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 106, no. 700, p. 619-625

Astronomy and Astrophysics

Astronomy

5

Infrared Spectra, Line Spectra, Planetary Nebulae, Ultraviolet Spectra, Visible Spectrum, Astronomical Spectroscopy, Contamination, Data Processing, Imaging Techniques, Spectral Resolution

Scientific paper

Observations of the planetary nebula Me 2-1 were obtained with different setups, in order to analyze some effects of contamination produced by the second-order ultraviolet spectrum in the first-order red, for wavelengths longer than approximately 6000 A. This contamination problem will be discussed elsewhere. Here we present the obervations of Me 2-1, which include a wide wavelength range, from about 3100 to 10,200 A. A comparison with previous results is shown for the wavelength intervals in common. From these data, the most relevant nebular parameters are derived, using lines in the optical and near IR regions. Some parameters corresponding to the central star are also determined. The results are compared with previously obtained values.

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