Chayan Mondal et al 2019 AJ 158 229
Far-ultraviolet imaging of the nearby dwarf irregular galaxy IC 2574 indicates that star formation in the galaxy is partly triggered due to expanding H I holes, but in most sites, it’s driven by other mechanisms.
C. Simpson et al 2019 ApJ 885 133
In the next stage of the Super-Kamiokande experiment, gadolinium sulfate will be added to the particle detector, potentially making it sensitive enough to be able to provide pre-explosion warnings for core-collapse supernovae.
Christina Kay et al 2019 ApJL 886 L37
Modeling based on the observationally reconstructed magnetic field of the 0.7 Gyr young Sun’s twin, k 1 Ceti, suggests that coronal mass ejections tend to propagate within a small cone about the ecliptic plane.
Lucas M. Macri et al 2019 ApJS 245 6
Redshifts are provided for all 1,041 Two Micron All-Sky Survey (2MASS) Redshift Survey galaxies that previously lacked this information due to their location in the Zone of Avoidance.
Stephen R. Kane and Sarah Blunt 2019 AJ 158 209
Despite the influence of the eccentric HR 5183 giant planet, there remain a narrow range of locations within the star’s habitable zone where terrestrial planets may reside in long-term stable orbits, dynamical simulations show.
Isidro Ramírez-Ballinas et al 2019 ApJ 885 116
Archival XMM-Newton observations of the diffuse X-ray emission from the star-forming region LMC-N 57 in the Large Magellanic Cloud unveils the powerful effect of massive stars in destroying their nurseries.