G. Tautvaišienė et al 2020 ApJS 248 19
New observations determine the main atmospheric parameters, ages, orbital parameters, velocity components, and chemical abundances for 277 slowly rotating single stars in the TESS continuous viewing zone field.
N. Rea et al 2020 ApJ 894 159
Chandra X-ray observations of SGR J1745−2900, a magnetar that lies within parsecs of the Milky Way’s central black hole Sgr A*, track its outburst onset in 2013 and subsequent cooling over the next 6 years.
Michaël Marsset et al 2020 Planet. Sci. J. 1 16
Examination of three binary trans-Neptunian objects show similar colors for each of the pairs, suggesting similar surface composition and supporting an origin model of gravitational collapse of a pebble cloud.
Colin J. Burke et al 2020 ApJL 894 L5
New Gemini spectroscopy of the blue compact dwarf galaxy PHL 293B reveals that its unusual broad emission lines have begun to fade after a decade of persistence, indicating they were likely due to a long-lived stellar transient.
Petr Pokorný et al 2020 ApJ 894 114
New analysis of regions within 5° of the two lunar poles shows that the poles are easily accessible by meteoroid impacts, including the permanently shadowed regions within deep lunar craters.
Veselin B. Kostov et al 2020 AJ 159 253
The Transiting Exoplanet Survey Satellite (TESS) has found its first planet orbiting around an eclipsing binary star system. The planet is ~6.9 Earth radii and has an orbital period of 95.2 days.