NASA NTRS · 19990063750
The Intermittently Embedded Herbig AE/BE Stars
Abstract
We discuss silicate emission profiles observed with the ISO SWS and ground-based IR observations in a population of intermittently embedded Herbig Ae/Be stars which are viewed edge-on to their polarimetrically identified dust and gas disks. The ISO SWS observations confirm the lack of a simple correlation between system age and the profile shape. Comparison with laboratory silicates suggests that much of the observed variation is due to different annealing histories of the grains.
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Grady, C. A., Perez, M. R., Bjorkman, K. S., Sitko, M. L., The, P. S., DeWinter, D., Grinin, V. P., Russell, R. W., Lynch, D. K., Hanner, M. S.. 1998-01-01. The Intermittently Embedded Herbig AE/BE Stars. https://ntrs.nasa.gov/citations/19990063750
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