ASPCS
 
Back to Volume
Paper: ISO Spectroscopy of Circumstellar Dust surrounding Isolated Herbig Ae/Be Stars
Volume: 196, Thermal Emission Spectroscopy and Analysis of Dust, Disks, and Regoliths
Page: 53
Authors: Waelkens, C.; Malfait, K.; Waters, L. B. F. M.; Meeus, G.
Abstract: 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.
Back to Volume