77 citations · 266 across the 6 of their papers we have counts for
6 papers
Effects of pebble accretion on the growth and composition of planetesimals in the inner Solar System
J. Mah, R. Brasser, A. Bouvier +1
Recent work has shown that aside from the classical view of collisions by increasingly massive planetesimals, the accretion of mm- to m-sized 'pebbles' can also reproduce the mass-…
How primordial is the structure of comet 67P/C-G? Combined collisional and dynamical models suggest a late formation
M. Jutzi, W. Benz, A. Toliou +2
There is an active debate about whether the properties of comets as observed today are primordial or, alternatively, if they are a result of collisional evolution or other processe…
Late veneer and late accretion to the terrestrial planets
R. Brasser, S. J. Mojzsis, S. C. Werner +2
It is generally accepted that silicate-metal (`rocky') planet formation relies on coagulation from a mixture of sub-Mars sized planetary embryos and (smaller) planetesimals that dy…
An updated estimate of the number of Jupiter-family comets using a simple fading law
R. Brasser, J. -H. Wang
It has long been hypothesised that the Jupiter-family comets (JFCs) come from the scattered disc, an unstable planetesimal population beyond Neptune. This viewpoint has been widely…
Reassessing the formation of the Inner Oort cloud in an embedded star cluster II: Probing the inner edge
R. Brasser, M. E. Schwamb
The detached object Sedna is likely at the inner edge of the Oort cloud, more precisely the inner Oort cloud (IOC). Until recently it was the sole member of this population. The re…
A dynamical study on the habitability of terrestrial exoplanets II: The super Earth HD 40307 g
R. Brasser, S. Ida, E. Kokubo
HARPS and it Kepler results indicate that half of solar-type stars host planets with periods P<100 d and masses M < 30 M_E. These super Earth systems are compact and dynamically co…