Aaron J. Barth et al 2016 ApJ 822 L28
NGC 1332 is used to demonstrate that by resolving gas kinematics on small angular scales in galaxy nuclei, ALMA is able to measure determine the masses of supermassive black holes.
A. Gianninas et al 2016 ApJ 822 L27
Three precursors to extremely low-mass white dwarfs with mixed H/He atmospheres were recently discovered to have asteroseismic pulsations, providing insight into what causes the pulsations.
F. Acero et al 2016 ApJS 224 8
The first systematic supernova remnant survey at energies from 1 to 100 GeV — using data from the Fermi Large Area Telescope (LAT) — reveals 30 sources as likely GeV supernova remnants.
Smadar Naoz et al 2016 ApJ 822 L24
Black hole low-mass X-ray binaries could form without a common-envelope phase and instead form via triple-body dynamics if they start out as a heierarchical triple star system.
S. Archambault et al 2016 AJ 151 142
Analysis of 114 blazars undetected by the VERITAS Cherenkov telescope array provides flux upper limits for these objects in the VERITAS energy band.
R. H. Cameron et al 2016 ApJ 823 L22
Surface flux transport simulations for solar Cycle 24 suggest the dipole moment in 2020 will be comparable to that at the end of Cycle 23. This argues that Cycle 25 may be moderate, like Cycle 24.