M. Meftah et al. 2015 ApJ 808 4

Does the Sun’s diameter vary as a function of time, and is it related to solar activity? Measurements taken during the rising phase of the current solar cycle suggest the answer is “no”.

Andrei Tokovinin et al. 2015 AJ 150 50

Speckle interferometric observations taken with the Southern Astrophysical Research Telescope provide measurements of 1218 resolved binary and multiple stars.

M. L. Parker et al. 2015 ApJ 808 9

NuSTAR and Suzaku spectra of the x-ray binary Cyg X-1 suggest the accretion disk around the black hole is not truncated in the hard state, but instead extends down to small radii.

Heather R. Jacobson et al. 2015 ApJ 807 171

The SkyMapper Southern Sky Survey, which seeks the most metal-poor stars in the Galaxy, has identified 122 low-metallicity stars in the Galactic halo and obtained high-resolution spectra for them.

Luca Izzo et al. 2015 ApJ 808 L14

Lithium was detected in spectra of nova V1369 Cen. Based on this observation, calculations suggest that classical novae could be one of the major Lithium producers on a Galactic scale.

R. Keppens et al. 2015 ApJ 806 L13

Simulations of the convective motions in solar prominences suggest that cool, dense chromospheric material is mixed into the prominence matter and carried to large heights.