Simulations require 2000 Earth masses of pebbles to match observed disc gaps, but this produces mostly gas giants and few super-Earths, contradicting exoplanet data.
N., Pierens A., 2013, @doi [ ] 10.1051/0004-6361/201220853 , http://adsabs.harvard.edu/abs/2013A
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.EP 1years
2019 1verdicts
UNVERDICTED 1representative citing papers
citing papers explorer
-
Are the observed gaps in protoplanetary discs caused by growing planets?
Simulations require 2000 Earth masses of pebbles to match observed disc gaps, but this produces mostly gas giants and few super-Earths, contradicting exoplanet data.