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20232026
most citedRetrograde discs around one component of a binary are unstable to tilting

6 citations · 15 across the 21 of their papers we have counts for

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Showing 2025 · astro-ph.EPShow all

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astro-ph.EP2025

Formation of super-Earths around low-mass stars: evolution of an icy dead zone

Danilo A. Arturo Rodriguez, Rebecca G. Martin

Exoplanet observations show that close-in super-Earths are more common around M-dwarfs than around solar mass stars. Since the snow line in a protoplanetary disc plays a crucial ro…

astro-ph.EP2025

Primordial planet spin driven by boundary layer effects in a decretion disc

Rebecca G. Martin, Stephen H. Lubow, David Vallet +4

Accretion of material from a protoplanetary disc on to a forming giant planet can spin the planet up to close to its breakup rate, , where $M_{…

astro-ph.EP2025

Planet-disc interactions around eccentric binaries and misaligned ring formation

Rebecca G. Martin, Stephen H. Lubow

We explore the evolution of a giant planet that interacts with a circumbinary disc that orbits a misaligned binary by means of analytic models and hydrodynamical simulations. Plane…

astro-ph.EP2025★ 2 cited

The fraction of polar aligned circumbinary disks

Ted M. Johnson, Rebecca G. Martin, Stephen Lepp +1

Circumbinary gas disks that are misaligned to the binary orbital plane evolve toward either a coplanar or a polar-aligned configuration with respect to the binary host. The preferr…

astro-ph.EP2025

Polar circumtriple planets and disks around misaligned hierarchical triple stars

Stephen Lepp, Rebecca G. Martin, Stephen H. Lubow

Observations of hierarchical triple star systems show that misalignments are common both between the angular momentum vector of the inner binary and the outer companion orbit, and…

astro-ph.EP2025

Observational Signatures of a Previous Dynamical Instability in Multi-planet M-Dwarf Systems

Anna C. Childs, Alexa P. S. Hua, Rebecca G. Martin +2

We identify observational signatures suggesting a history of dynamical instability in 26 out of 34 M-dwarf multi-planet systems containing no large planets. These systems may have…