Herbig Ae/Be stars: Fine structure far-infrared lines

Details Herbig Ae/Be stars: Fine structure far-infrared lines Herbig Ae/Be stars: Fine structure far-infrared lines

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.290..343c&link_type=abstract

In ESA, Infrared Spectroscopy in Astronomy p 343-349 (SEE N90-19084 11-89)

Astronomy and Astrophysics

Astronomy

1

Far Infrared Radiation, Fine Structure, Herbig-Haro Objects, Spaceborne Astronomy, Spectrum Analysis, Stellar Radiation, Emission Spectra, European Space Programs, Infrared Astronomy, Infrared Space Observatory (Iso), Line Spectra, Stellar Spectra

Scientific paper

The preliminary results on the far infrared fine structure lines in the partially ionized regions around Herbig Ae/Be stars, are presented. An interpretation model is proposed. The main contributions to heating and cooling on a grid of spherical zones, allows an estimate of the line fluxes. The results are compared with the sensitivity of the long wavelength spectrometer on board the future ESA Infrared Space Observatory satellite.

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