Conference
Physics and Astrophysics of Dust II
Book
Dust sources
evolved stellar
SN
QSO
Dust evolution in ISM
dust destruction
dust growth
Interstellar Dust Models
At this point, it is not possible to “invert” the observations to “derive” the nature of interstellar dust – neither theory nor observations are good enough. The only feasible approach is to propose a dust model, calculate its properties, and compare it to observations. If the model disagrees with the observations, it is rejected. (Draine, B.T.2004)
dust composition
Size distribution
Reddening
科普
Smoking Supernovae
At this point, it is not possible to “invert” the observations to “derive” the
nature of interstellar dust – neither theory nor observations are good enough.
The only feasible approach is to propose a dust model, calculate its properties,
and compare it to observations. If the model disagrees with the observations, it
is rejectedAt this point, it is not possible to “invert” the observations to “derive” the
nature of interstellar dust – neither theory nor observations are good enough.
The only feasible approach is to propose a dust model, calculate its properties,
and compare it to observations. If the model disagrees with the observations, it
is rejected.
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