Tomoharu Oka et al 2016 ApJ 816 L7
The motion of the high-velocity compact cloud CO–0.40–0.22 is proposed to be due to a gravitational kick from an intermediate-mass (10^5 solar masses) black hole located in our galaxy’s CMZ.
C. M. Lisse et al 2015 ApJ 815 L27
New observations of the star KIC 8462852, which exhibits unusual dips in its lightcurve, suggest that the system may actually be in the early stages of a late heavy bombardment.
J. A. Rich et al 2015 ApJS 221 28
A study of radiative shocks in 27 nearby ultraluminous and luminous infrared galaxies indicate that more and more emission is driven by shocks as the galaxy merger stage progresses.
D. Perna et al 2016 AJ 151 11
Spectroscopic observations of 14 Potentially Hazardous Asteroids (PHAs) are used, along with past literature, to analyze the distribution of PHAs as a function of their dynamical and physical properties.
Amber N. Straughn et al 2015 ApJ 814 97
Multiwavelength studies of galaxies with distinct asymmetric knot-plus-tail morphologies in the Hubble Ultra Deep Field suggest that these “tadpole” galaxies may be in an active phase of assembly.
M. L. Ahnen et al 2015 ApJ 815 L23
Corresponding MAGIC detection of PKS 1441+25’s gamma-ray outburst: emission originates in the jet from outside the broad line region (BLR) during high activity and from within the BLR during low activity.