Bei You et al 2016 ApJ 821 104
One issue with the continuum-fitting method for estimating black-hole spin is the apparent decrease in spin with increasing source luminosity. This can be resolved by assuming the presence of a disk wind.
S. Renner et al 2016 AJ 151 122
Saturn’s moon Atlas exhibits a chaotic orbit whose dynamics are primarily controlled by resonant perturbations from the moon Prometheus. This may be common in satellite evolution around giant planets.
S. Heinis et al 2016 ApJ 821 86
A set of machine-learning tools are shown to be useful for automatically differentiating between stars and galaxies in large survey catalogs, and also for estimating photometric redshifts of galaxies.
F. Bernardini et al 2016 ApJ 818 L5
Optical observations of V404 Cyg prior to its X-ray outburst suggest this black hole’s disk entered the hot, outburst state before the X-ray outburst. The event may have been triggered by a disk instability.
M. Kounkel et al 2016 ApJ 821 52
NIR Hubble observations of Orion molecular clouds reveal that the fraction of stars with 100-1000 AU companions is ~50% higher in the high-stellar-density regions, relative to the low-density regions.
P. Narayana Bhat et al 2016 ApJS 223 28
The Fermi Gamma-ray Burst Monitor locates an average of ~2 gamma-ray burst events every 3 days. The catalog of these events, spanning 2008 to 2014, contains 1405 triggers identified as GRBs.