Interstellar Medium (ISM) - Gas and Dust

Carina Nebula ImageCarina Nebula


Interstellar Medium:

Dust

Measurement:
Extinction (including red shift) of Electromagnetic Radiation
Polarization of light

Gas

Measurement:
Radio Emission (molecules)
Radio Absorption (21 cm)
Optical Absorption
Type of ISM Comment Density
(Molecules/cm3)
Temperature (K) Mass (MSun) Size (ly)
Cold Atomic Atomic Hydrogen
In Equilibrium
10-20 50 1000 30
mean separation 500ly
Warm Atomic Atomic Hydrogen
In equilibrium
0.1 5000 This and Cold make 50% of all ISM Mass Small Fraction of Volume
Coronal Gas Typical of Solar Area
Heated by Supernova
0.01 1,000,000 very small 50% of all volume
Molecular Clouds H2 not detectible
CO radiation used to map locations
Not in gravitational equilibrium
1000-10,000 ~10 ~<1,000,000
50% of ISM mass!
50-100
(< 1% of space)
HII Regions associated with Molecular Clouds
Hot and expanding
100-1000 10,000 Small fraction Small fraction of volume