Electronic Resource
Springer
Astrophysics and space science
271 (2000), S. 259-276
ISSN:
1572-946X
Source:
Springer Online Journal Archives 1860-2000
Topics:
Physics
Notes:
Abstract IRAS low-resolution spectra are presented for 36 HAEBE stars. It is found that silicate dust is common material in the circumstellar disks or/and shells of HAEBE stars. It is also found that the PAH feature often appears as well. In addition, the correlation between the dust features and spectral type, and infrared excesses can be found for most HAEBE stars.
Type of Medium:
Electronic Resource
URL:
http://dx.doi.org/10.1023/A:1002405302952
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