activity
20052026
most citedBinary interaction dominates the evolution of massive stars

2.1k citations · 6.7k across the 89 of their papers we have counts for

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Showing 2018Show all

6 papers · 1 filter

astro-ph.SR2018★ 27 cited

Probing the Inner Disk Emission of the Herbig Ae Stars HD 163296 and HD 190073

Benjamin R. Setterholm, John D. Monnier, Claire L. Davies +16

The physical processes occurring within the inner few astronomical units of proto-planetary disks surrounding Herbig Ae stars are crucial to setting the environment in which the ou…

astro-ph.GA2018★ 431 cited

Detection of orbital motions near the last stable circular orbit of the massive black hole SgrA*

GRAVITY Collaboration, R. Abuter, A. Amorim +57

We report the detection of continuous positional and polarization changes of the compact source SgrA* in high states ('flares') of its variable near- infrared emission with the nea…

astro-ph.SR2018★ 38 cited

Multiple Star Systems in the Orion Nebula

GRAVITY collaboration, Martina Karl, Oliver Pfuhl +133

This work presents an interferometric study of the massive-binary fraction in the Orion Trapezium Cluster with the recently comissioned GRAVITY instrument. We observe a total of 16…

astro-ph.SR2018★ 3 cited

GRAVITY chromatic imaging of Eta Car's core

GRAVITY Collaboration, J. Sanchez-Bermudez, G. Weigelt +132

Eta Car is one of the most intriguing luminous blue variables in the Galaxy. Observations and models at different wavelengths suggest a central binary with a 5.54 yr period residin…

astro-ph.GA2018★ 947 cited

Detection of the gravitational redshift in the orbit of the star S2 near the Galactic centre massive black hole

GRAVITY Collaboration, R. Abuter, A. Amorim +95

The highly elliptical, 16-year-period orbit of the star S2 around the massive black hole candidate Sgr A* is a sensitive probe of the gravitational field in the Galactic centre. Ne…

astro-ph.SR2018★ 20 cited

Dynamical masses of M-dwarf binaries in young moving groups: I - The case of TWA 22 and GJ 2060

L. Rodet, M. Bonnefoy, S. Durkan +48

Evolutionary models are widely used to infer the mass of stars, brown dwarfs, and giant planets. Their predictions are thought to be less reliable at young ages ( 200 Myr) and i…