Search Results - "Wimarsson, John"
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1
Promoted mass growth of multiple, distant giant planets through pebble accretion and planet–planet collision
Published in Monthly notices of the Royal Astronomical Society (11-08-2020)“…ABSTRACT We propose a pebble-driven planet formation scenario to form giant planets with high multiplicity and large orbital distances in the early gas disc…”
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2
The velocity distribution of white dwarfs in Gaia EDR3
Published in Monthly notices of the Royal Astronomical Society (20-04-2022)“…ABSTRACT Using a penalized maximum likelihood, we estimate, for the first time, the velocity distribution of white dwarfs in the solar neighbourhood. Our…”
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3
Rapid formation of binary asteroid systems post rotational failure: A recipe for making atypically shaped satellites
Published in Icarus (New York, N.Y. 1962) (01-10-2024)“…Binary asteroid formation is a highly complex process, which has been highlighted with recent observations of satellites with unexpected shapes, such as the…”
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The Dynamical State of the Didymos System before and after the DART Impact
Published in The planetary science journal (2024)“…NASA’s Double Asteroid Redirection Test (DART) spacecraft impacted Dimorphos, the natural satellite of (65803) Didymos, on 2022 September 26, as a first…”
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5
Rapid formation of binary asteroid systems post rotational failure: a recipe for making atypically shaped satellites
Published 22-07-2024“…Binary asteroid formation is a highly complex process, which has been highlighted with recent observations of satellites with unexpected shapes, such as the…”
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Journal Article -
6
The velocity distribution of white dwarfs in Gaia EDR3
Published 15-02-2022“…Using a penalised maximum likelihood we estimate, for the first time, the velocity distribution of white dwarfs in the Solar neighbourhood. Our sample consists…”
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Journal Article -
7
Promoted Mass Growth of Multiple, Distant Giant Planets through Pebble Accretion and Planet-Planet Collision
Published 11-06-2020“…We propose a pebble-driven planet formation scenario to form giant planets with high multiplicity and large orbital distances in the early gas disk phase. We…”
Get full text
Journal Article