N. Scoville et al 2017 ApJ 837 150

ALMA observations of the dust continuum in 700 galaxies at z = 0.3–4.5 indicate that increases in star formation at high z are due to both increased ISM masses and increased gas-to-star conversion efficiency.

Stelios Kazantzidis et al 2017 ApJL 836 L13

The combination of ram-pressure stripping and supernova winds causes tidal stirring to be an effective and prevalent mechanism for shaping the structure of dwarf galaxies within CDM cosmology.

M. Soto et al 2017 AJ 153 19

A new catalog of 57 globular clusters — built from an early release of HST Treasury survey data — is intended for use in identifying stars in different stellar populations, in particular for spectroscopic follow-up.

Jeremy Darling 2017 ApJ 837 100

Inclined water maser disks can be identified by searching for narrow masers near the systemic velocity that appear to emit from the position of the central black hole that they orbit.

Shugo Michikoshi and Eiichiro Kokubo 2017 ApJL 837 L13

Global N-body simulations of self-gravitating collisional particle rings indicate that the Centaur Chariklo must be even denser than the material of its two rings, which would generate wakes in its inner ring.

Duane F. Carbon et al 2017 ApJS 228 19

A new search approach for large spectrum data sets found 59 new extremely metal-poor stars, 11 new carbon-enhanced metal-poor stars, and 2 new cataclysmic variable stars in the SDSS DR10 data set.