ISO Spectroscopy of Circumstellar Dust surrounding Isolated Herbig Ae/Be Stars

Details ISO Spectroscopy of Circumstellar Dust surrounding Isolated Herbig Ae/Be Stars ISO Spectroscopy of Circumstellar Dust surrounding Isolated Herbig Ae/Be Stars

Mar 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aspc..196...53w&link_type=abstract

Thermal Emission Spectroscopy and Analysis of Dust, Disks, and Regoliths, Proceedings of a meeting held at at The Lunar and Plan

Astronomy and Astrophysics

Astronomy

6

Scientific paper

Herbig Ae/Be stars -- hereafter HAEBE stars -- are assumed to be the evolutionary precursors of Vegalike stars. In isolated HAEBE stars the IR excess is produced uniquely by the circumstellar disk which can be seen as an early evolutionary stage of a forming planetary system. We present and discuss ISO spectra of isolated HAEBE stars, with the aim of identifying the main dust components and linking them with observations of solar-system dust.

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