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The Interstellar Medium. ISM Properties - 99% is gas, mostly H, He - about 1 atom/cm 3 - 1% is dust grains, mostly C, ices of water, ammonia, methane - 10 -6 meters in diameter - about 1 grain/100m 3. ISM Properties (continued) - Temps between 5K to 10,000K near hot stars
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ISM Properties - 99% is gas, mostly H, He - about 1 atom/cm3 - 1% is dust grains, mostly C, ices of water, ammonia, methane - 10-6 meters in diameter - about 1 grain/100m3
ISM Properties (continued) - Temps between 5K to 10,000K near hot stars - About 10% of the mass of our Galaxy is ISM
HII regions - ionized regions around hot stars Ionized H (HII) Hot O,B star
30 Doradus (Trantula Nebula)
The ISM absorbs short wavelengths more than long ones -> the ISM reddens and dims starlight
21-cm Radiation H-Atom Low energy High Energy 21 cm photon
Nebulae (clouds) - Concentrations in the ISM (1,000’s of atoms/cm3) - The building blocks of the Stars
Dark Nebulae - lots of Dust Horsehead Nebula
Reflection Nebulae - shine by reflected light from nearby stars Witch Head Nebula