Philipp Girichidis et al 2016 ApJ 816 L19
MHD simulations of supernova-driven interstellar medium show that cosmic rays are able to launch and sustain strong outflows of atomic and ionized gas, with mass-loading factors of ~1.
Jason H. Steffen and Gongjie Li 2016 ApJ 816 97
Numerical simulations of resonant planet-planet interactions show that close-proximity pairs of planets that lie in their host’s habitable zone can be conducive to life in the system.
Sarah Ballard and John Asher Johnson 2016 ApJ 816 66
The best model of Kepler M-dwarf planet hosts predicts that roughly half of these hosts contain ~7 coplanar planets. The other half contain single planets, or multiple planets with large mutual inclinations.
Andrew J. Fox et al 2016 ApJ 816 L11
Hubble measurements show that the Smith Cloud is metal-enriched, suggesting it represents recycled Galactic material rather than a dwarf galaxy remnant or accreting intergalactic gas.
Jason Galyardt and Robin L. Shelton 2016 ApJ 816 L18
If the Smith high velocity cloud has a dark-matter minihalo, simulations suggest the cloud’s gas was accreted in a collision with the Galactic disk. If it’s dark matter free, then this is the cloud’s first approach.
Ing-Guey Jiang et al 2016 AJ 151 17
New data and analysis finds an orbital decay rate for the short-period exoplanet WASP-43b of ~0.029 s/yr, an order of magnitude lower than previously reported rates.