activity
20022026
most citedDisk-mediated accretion burst in a high-mass young stellar object

231 citations · 3.5k across the 145 of their papers we have counts for

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Showing 2018Show all

8 papers · 1 filter

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★ 15 cited

Photometric variability of massive young stellar objects. I

G. D. C. Teixeira, M. S. N. Kumar, L. Smith +8

The VVV survey has allowed for an unprecedented number of multi-epoch observations of the southern Galactic plane. In a recent paper,13 massive young stellar objects(MYSOs) have al…

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.SR2018★ 1 cited

Supersize me! Jets from massive young stellar objects

Alessio Caratti o Garatti

This short review examines the most recent observational results obtained for jets driven by high-mass young stellar objects (HMYSOs). Reviewed data range from near-infrared to rad…

astro-ph.SR2018★ 19 cited

Parsec-scale jets driven by high-mass young stellar objects. Connecting the au- and the parsec-scale jet in IRAS 13481-6124

R. Fedriani, A. Caratti o Garatti, D. Coffey +6

Context: Protostellar jets in high-mass young stellar objects (HMYSOs) play a key role in the understanding of star formation and provide us with an excellent tool to study fundame…

astro-ph.SR2018★ 4 cited

The circumstellar environment of HD50138 revealed by VLTI/AMBER at high angular resolution

M. Koutoulaki, R. Garcia Lopez, A. Natta +4

HD50138 is a Herbig B[e] star with a circumstellar disc detected at IR and mm wavelength. Its brightness makes it a good candidate for NIR interferometry observations. We aim to re…