Stephen Durkan et al 2016 ApJ 824 58

Re-analysis of archival Spitzer IRAC surveys indicate that the frequency of 0.5–13 Jupiter-mass planets at separations of 10–1000 AU is less than 9% in the study sample.

Kumiko Kotera and Joseph Silk 2016 ApJ 823 L29

If merging black holes like those in LIGO detection GW140915 have spin, relic magnetic fields, and surrounding disk debris, the merger environment could accelerate ultrahigh-energy cosmic rays.

Luke D. Burkhart et al 2016 AJ 151 162

Hubble observations are used to search for new very small satellites of Haumea, a dwarf planet with two known satellites. Satellites similar in size to the small moons of Pluto are ruled out.

D. Crnojević et al 2016 ApJ 823 19

A wide-field stellar map of Cen A (a close massive elliptical galaxy) reveals previously unknown streams, shells, and 13 dwarf satellite candidates, including the first tidally disrupting dwarf found around Cen A.

Ryo Suetsugu et al 2016 AJ 151 140

Planetesimals captured by disks around gas giants typically spiral rapidly into the planet. Planetesimal orbits that are initially retrograde decay faster, and high gas drag can turn them to prograde orbits.

Lucio Mayer et al 2016 ApJ 823 L36

3D simulations of protoplanetary disks show that ALMA has the capability to detect the overdense spiral arms and clumps representing precursors to the formation of gas giant planets.