Mid-infrared spectroscopy of protoplanetary and planetary nebulae

Details Mid-infrared spectroscopy of protoplanetary and planetary nebulae Mid-infrared spectroscopy of protoplanetary and planetary nebulae

Oct 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002mnras.336...66r&link_type=abstract

Monthly Notice of the Royal Astronomical Society, Volume 336, Issue 1, pp. 66-72.

Astronomy and Astrophysics

Astronomy

5

Astrochemistry, Techniques: Spectroscopic, Ism: Lines And Bands, Planetary Nebulae: General, Infrared: Ism

Scientific paper

We present medium-resolution (R~ 600), mid-infrared (7.5-14 μm)
spectra of 15 young planetary nebulae. Linestrengths for observed
forbidden transitions are presented, and numerous broad emission
features from silicates, polyaromatic hydrocarbons (PAHs) and silicon
carbide (SiC) are observed.

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