SIMBAD references

2004ApJ...612.1147K - Astrophys. J., 612, 1147-1151 (2004/September-2)

A minimum-mass extrasolar nebula.

KUCHNER M.J.

Abstract (from CDS):

By analogy with the minimum-mass solar nebula, we construct a surface-density profile using the orbits of the 26 precise-Doppler planets found in multiple-planet systems: Σ=2200(a/1AU)–βg/cm2, where a is the circumstellar radius and β=2.0±0.5. The minimum-mass solar nebula (β=1.5) is consistent with this model, but the uniform-α accretion disk model (β~1) is not. In a nebula with β>2, the center of the disk is the likely cradle of planet formation.

Abstract Copyright:

Journal keyword(s): Stars: Planetary Systems: Protoplanetary Disks - Solar System: Formation

Simbad objects: 17

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2019.09.19-09:11:03

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