Global N-body simulations of circumbinary planet formation around Kepler-16 and -34 analogues I: Exploring the pebble accretion scenario (2023)
Attributed to:
Astronomy Research at Queen Mary
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2303.09899
Publication URI: https://arxiv.org/abs/2303.09899
Type: Other