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Self-similarity and scaling behavior of IR emission from radiatively heated dust: I. Theory
Zeljko Ivezic, Moshe Elitzur
Dust infrared emission possesses scaling properties. Overall luminosity is never an input parameter of the radiative transfer problem, spectral shape is the only relevant property…
On Protostellar Disks in Herbig Ae/Be Stars
Anatoly Miroshnichenko, Zeljko Ivezic, Moshe Elitzur
The spectral shape of IR emission from Herbig Ae/Be stars has been invoked as evidence for accretion disks around high-mass protostars. Instead, we present here models based on sph…
IR Emission from dusty winds --- Scaling and self-similarity properties
Moshe Elitzur, Zeljko Ivezic
Infrared emission from radiatively heated dust possesses general scaling properties. The spectral shape is independent of overall luminosity when the inner boundary of the dusty re…
Infrared Imaging of Late-Type Stars
Zeljko Ivezic, Moshe Elitzur
Infrared imaging properties of dusty winds around late-type stars are investigated in detail, employing a self-consistent model that couples the equations of motion and radiative t…
Dust Emission from IRC+10216
Zeljko Ivezic, Moshe Elitzur
Infrared emission from the dust shell around IRC+10216 is analysed in detail, employing a self-consistent model for radiatively driven winds around late-type stars that couples the…