ABSTRACT

Interstellar dust grains catalyse chemical reactions, absorb, scatter, polarise and re-radiate starlight and constitute the building blocks for the formation of planets. Understanding this interstellar component is therefore of primary importance in many areas of astronomy & astrophysics. For example, observers need to understand how dust effects l

chapter Chapter 1|43 pages

The dielectric permeability

chapter Chapter 2|36 pages

How to evaluate grain cross sections

chapter Chapter 3|38 pages

Very small and very big particles

chapter Chapter 4|26 pages

Case studies of Mie calculus

chapter Chapter 5|30 pages

Particle statistics

chapter Chapter 6|26 pages

The radiative transition probability

chapter Chapter 7|38 pages

Structure and composition of dust

chapter Chapter 8|36 pages

Dust radiation

chapter Chapter 9|44 pages

Dust and its environment

chapter Chapter 10|28 pages

Polarization

chapter Chapter 11|30 pages

Grain alignment

chapter Chapter 12|19 pages

PAHs and spectral features of dust

chapter Chapter 13|29 pages

Radiative transport

chapter Chapter 14|36 pages

Diffuse matter in the Milky Way

chapter Chapter 15|45 pages

Stars and their formation

chapter Chapter 16|34 pages

Emission from young stars