Dust

Conference

Astrophysics of Dust

Physics and Astrophysics of Dust II

Cosmic Dust – Near and Far

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.