activity
20142024
most citedConsequences of a Distant Massive Planet on the Large Semi-major Axis Trans-Neptunian Objects

41 citations · 192 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.EP2024

Satellite Visibility During the April 2024 Total Eclipse

Samantha M. Lawler, Hanno Rein, Aaron C. Boley

On 8 April 2024, tens of millions of people across North America will be able to view a total solar eclipse. Such astronomical events have been important throughout history, but wi…

astro-ph.SR202213 cited

Investigating the stability of mass transfer in neutron star-helium white dwarf binaries

Hai-Liang Chen, Thomas M. Tauris, Xuefei Chen +1

Neutron star-helium white dwarf (NS+He WD) binaries are important evolutionary products of close-orbit binary star systems. They are often observed as millisecond pulsars and may c…

astro-ph.EP201641 cited

Consequences of a Distant Massive Planet on the Large Semi-major Axis Trans-Neptunian Objects

C. Shankman, JJ Kavelaars, S. M. Lawler +2

We explore the distant giant planet hypothesis by integrating the large semi-major axis, large pericenter Trans-Neptunian Objects (TNOs) in the presence of the giant planets and an…

astro-ph.SR201634 cited

ALMA Observations of the Debris Disk of Solar Analogue Tau Ceti

Meredith A. MacGregor, Samantha M. Lawler, David J. Wilner +4

We present 1.3 mm observations of the Sun-like star Ceti with the Atacama Large Millimeter/submillimeter Array (ALMA) that probe angular scales of '' (4 AU). This first…

astro-ph.EP201620 cited

OSSOS: IV. Discovery of a dwarf planet candidate in the 9:2 resonance with Neptune

Michele T. Bannister, Mike Alexandersen, Susan D. Benecchi +32

We report the discovery and orbit of a new dwarf planet candidate, 2015 RR, by the Outer Solar System Origins Survey (OSSOS). 2015 RR's orbit is eccentric ($e=0.586…

astro-ph.EP201441 cited

Fomalhaut b as a Dust Cloud: Frequent Collisions within the Fomalhaut Disk

S. M. Lawler, S. Greenstreet, B. Gladman

The planet candidate Fomalhaut b is bright in optical light but undetected in longer wavelengths, requiring a large, reflective dust cloud. The most recent observations find an ext…