PX282 - L1 - nebular hypothesis

PX282 - L1 - nebular hypothesis.png|500
image: R. Townsend, UCL

Σ(r)∝r−3/2

where, Σ is the surface density of the disc ([kg m2])

Mdisc≥0.01M⊙ Tdisc∝r−3/4

PX282 - L1 - nebular hypothesis-1.png|500
image: Hayashi (1989), D. Forgan

PX282 - L1 - nebular hypothesis-2.png|500
image: IAU