Markus Janson et al 2016 ApJ 816 L1
A newly detected feature in the scattered-light image of the circumbinary disk around the young double star AK Sco may be an eccentric ring or spiral arms, possibly caused by an orbiting planet.
K. I. I. Koljonen et al 2015 ApJ 814 139
The properties of jets produced by black holes may be primarily dependent on the properties of the plasma near the black hole, rather than on parameters like the black hole’s mass or spin.
A. Richichi et al 2016 AJ 151 10
Observations of the Moon occulting 18 stellar sources led to the detection of four angular diameters and two binary stars. Resolution limits of this study were 2 mas for diameters and 4 mas for separations.
Paul A. Dalba et al 2015 ApJ 814 154
This study explores the 1–5 micrometer transmission spectrum of Saturn as though it were a transiting exoplanet, using observations from the spectrometer on board the Cassini spacecraft.
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.