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20052026
most citedFirst Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way

1.9k citations · 17.5k across the 156 of their papers we have counts for

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astro-ph.SR2024

Deep JWST/NIRCam imaging of Supernova 1987A

Mikako Matsuura, M. Boyer, Richard G. Arendt +46

JWST/NIRCam obtained high angular-resolution (0.05-0.1''), deep near-infrared 1--5 micron imaging of Supernova (SN) 1987A taken 35 years after the explosion. In the NIRCam images,…

astro-ph.SR2019★ 7 cited

Evidence of a substellar companion to AB Dor C

J. B. Climent, J. P. Berger, J. C. Guirado +5

Studies of fundamental parameters of very low-mass objects are indispensable to provide tests of stellar evolution models that are used to derive theoretical masses of brown dwarfs…

astro-ph.SR2018★ 17 cited

Molecular line study of the S-type AGB star W Aquilae. ALMA observations of CS, SiS, SiO and HCN

Magdalena Brunner, Taissa Danilovich, Sofia Ramstedt +5

Context. With the outstanding spatial resolution and sensitivity of the Atacama Large Millimeter/sub-millimeter Array (ALMA), molecular gas other than the abundant CO can be observ…

astro-ph.SR2017★ 43 cited

Magnetically aligned dust and SiO maser polarization in the envelope of the red supergiant VY CMa

W. H. T. Vlemmings, T. Khouri, I. Marti-Vidal +9

We use Atacama Large Millimeter/submillimeter Array Band 5 science verification observations of the red supergiant VY CMa to study the polarization of SiO thermal/masers lines and…

astro-ph.SR2017★ 3 cited

Young, active radio stars in the AB Doradus moving group

R. Azulay, J. C. Guirado, J. M. Marcaide +5

Context. Precise determination of stellar masses is necessary to test the validity of pre-main-sequence (PMS) stellar evolutionary models, whose predictions are in disagreement wit…

astro-ph.SR2015★ 18 cited

Dynamical masses of the low-mass stellar binary ABDoradusB

R. Azulay, J. C. Guirado, J. M. Marcaide +8

Context. ABDoradus is the main system of the ABDoradus moving group. It is a quadruple system formed by two widely separated binaries of pre-main-sequence (PMS) stars: ABDor A/C an…