IDS spectroscopy of planetary nebulae

Details IDS spectroscopy of planetary nebulae IDS spectroscopy of planetary nebulae

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987msngr..48...16a&link_type=abstract

ESO Messenger (ISSN 0722-6691), June 1987, v. 48, p. 16-19.

Astronomy and Astrophysics

Astronomy

8

Astronomical Spectroscopy, Emission Spectra, Line Spectra, Planetary Nebulae, Data Reduction, Error Analysis, Luminosity, Milky Way Galaxy, Southern Sky, Spectrum Analysis

Scientific paper

Observations of planetary nebulae performed with the image dissecting scanner (IDS) of the 1.52-m telescope at La Silla are discussed. The quality of the IDS data is analyzed with attention given to reliability, measurement of blends, and the nonlinearity of the IDS system. Misclassified planetary nebulae are identified and some physical properties of planetary nebulae are determined.

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