Nebula — Stellar Nursery
Radiative MHD · Photoionisation · Shock Physics
H-α emission — ionised hydrogen
OIII — doubly ionised oxygen
dust lanes — extinction columns
protostellar cores — YSO jets
shock fronts — Rayleigh-Taylor

distance ~1.34 kpc

T_ion 8 000 K

n_e 100 cm⁻³

B_field ~30 μG

E_turb σ_v ≈ 4 km/s

age ~3 Myr

All
Ionised
Dust
Stars
Shocks

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Photoionisation
Strömgren sphere
UV photons from OB stars ionise H. Recombination emits H-α 656 nm. Lyman-α trapped.
MHD Turbulence
Alfvén waves
Magnetic pressure B²/8π. Kolmogorov cascade P(k)∝k⁻⁵/³. Ambipolar diffusion.
Shock Physics
Rankine-Hugoniot
Mach 5–40 shocks. Rayleigh-Taylor instability. Kelvin-Helmholtz pillars. SiO maser.
Dust Extinction
A_V ~ 1–30 mag
Silicate & carbonaceous grains. κ_ν ∝ ν^β, β≈2. FIR re-emission. PAH bands.
Star Formation
Jeans mass M_J
Dense cores collapse. Protostellar jets (v~200 km/s). Herbig-Haro objects. IMF.
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