output
19922026
most citedObservation of Gravitational Waves from a Binary Black Hole Merger

14.2k citations

Showing 2016 · astro-ph.SRShow all

8 papers · 2 filters

astro-ph.SR2016★ 231 cited

The MiMeS survey of magnetism in massive stars: Magnetic analysis of the O-type stars

J. H. Grunhut, G. A. Wade, C. Neiner +9

We present the analysis performed on spectropolarimetric data of 97 O-type targets included in the framework of the MiMeS (Magnetism in Massive Stars) Survey. Mean Least-Squares De…

astro-ph.SR2016★ 20 cited

HD 164492C: a rapidly-rotating, H-bright, magnetic early B star associated with a 12.5d spectroscopic binary

G. A. Wade, M. Shultz, J. Sikora +6

We employ high resolution spectroscopy and spectropolarimetry to derive the physical properties and magnetic characteristics of the multiple system HD 164492C, located in the young…

astro-ph.SR2016★ 32 cited

Dynamical Mass Measurement of the Young Spectroscopic Binary V343 Normae AaAb Resolved With the Gemini Planet Imager

Eric L. Nielsen, Robert J. De Rosa, Jason Wang +44

We present new spatially resolved astrometry and photometry from the Gemini Planet Imager of the inner binary of the young multiple star system V343 Normae, which is a member of th…

astro-ph.SR2016★ 42 cited

An active, asynchronous companion to a redback millisecond pulsar

André van Staden, John Antoniadis

PSR\,J17232837 is a "redback" millisecond pulsar (MSP) with a low-mass companion in a 14.8\,h orbit. The system's properties closely resemble those of "transitional" MSPs that a…

astro-ph.SR2016★ 4 cited

Stellar atmospheres, atmospheric extension and fundamental parameters: weighing stars using the stellar mass index

Hilding R. Neilson, Fabien Baron, Ryan Norris +2

One of the great challenges in understanding stars is measuring their masses. The best methods for measuring stellar masses include binary interaction, asteroseismology and stellar…

astro-ph.SR2016★ 32 cited

Chemical Abundances in a Sample of Red Giants in the Open Cluster NGC 2420 from APOGEE

Diogo Souto, Katia Cunha, Verne Smith +20

NGC 2420 is a 2 Gyr-old well-populated open cluster that lies about 2 kpc beyond the solar circle, in the general direction of the Galactic anti-center. Most previous abundan…