Dust in planetary nebulae: IRSPEC observations in the 3.0 micron-3.8 micron range

Details Dust in planetary nebulae: IRSPEC observations in the 3.0 micron-3.8 micron range Dust in planetary nebulae: IRSPEC observations in the 3.0 micron-3.8 micron range

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.290..371m&link_type=abstract

In ESA, Infrared Spectroscopy in Astronomy p 371-373 (SEE N90-19084 11-89)

Astronomy and Astrophysics

Astronomy

5

Infrared Astronomy, Infrared Spectroscopy, Interplanetary Dust, Planetary Nebulae, Spectral Line Width, Infrared Spectra, Infrared Spectrometers, Radiant Flux Density, Spectral Resolution, Spectrophotometers, Spectrum Analysis, Stellar Models

Scientific paper

The observations of eight planetary nebulae carried out with the infrared spectrometer, IRSPEC, in the range of 3.0 to 3.8 microns, are reported. They were collected in June 1988 at the European Southern Observatory (Chile) and were performed in a continuous mode with a spectral resolution of about 1100. In the infrared spectra, the unidentified infrared features are observed and discussed in the light of theories concerning dust grain properties. Photometric standard stars are observed in order to data calibrate in flux units.

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