Anthony L. Piro and Sarah Burke-Spolaor 2017 ApJL 841 L30
Modeling suggests two fast radio bursts detected within 9 arcmin of each other over 3 years apart could have been both caused by a supernova that occurred within ~10.2 years of FRB 110220.
Huidong Hu et al 2017 ApJ 840 76
Extreme ultraviolet imaging, magnetogram, white-light, and in situ observations from SDO, STEREO, SOHO, VEX, and Wind reveal the dynamics and evolution of a CME ejected from an area linking two active regions.
Samantha K. Trumbo et al 2017 AJ 153 250
Near-infrared spectroscopy of the surface of Europa revealed a previously unseen spectral feature in the trailing hemisphere consistent with that of a radiolytic product created by electron or ion bombardment.
Chao He et al 2017 ApJL 841 L31
Planetary atmosphere simulation experiments reveal that changing initial levels of CO in planetary atmospheres affects the gas phase chemistry, the density, and the composition of the solids.
F. Acero et al 2017 ApJ 840 74
Simulations are presented for future Cherenkov Telescope Array observations of RX J1713.7−3946, a young supernova remnant, to demonstrate how to distinguish the emission mechanisms of the gamma rays.
Mathias Ross and Vikram V. Dwarkadas 2017 AJ 153 246
The Supernova X-ray Database (SNaX) is a compilation of the X-ray data from young supernovae, from days to years after outburst. SNaX provides public access to the data and plot for each supernova.