activity
20072019
most citedA Likely Close-In Low-Mass Stellar Companion to the Transitional Disk Star HD 142527

184 citations · 1.7k across the 26 of their papers we have counts for

collaborators

26 papers

astro-ph.EP2019★ 50 cited

New millimeter CO observations of the gas-rich debris disks 49 Cet and HD 32297

Attila Moór, Quentin Kral, Péter Ábrahám +7

Previous observations revealed the existence of CO gas at nearly protoplanetary level in several dust-rich debris disks around young A-type stars. Here we used the ALMA 7m-array to…

astro-ph.SR2018★ 38 cited

VLTI/MIDI atlas of disks around low- and intermediate-mass young stellar objects

J. Varga, P. Ábrahám, L. Chen +13

Context. Protoplanetary disks show large diversity regarding their morphology and dust composition. With mid-infrared interferometry the thermal emission of disks can be spatially…

astro-ph.SR2017★ 117 cited

Signatures of broken protoplanetary discs in scattered light and in sub-millimetre observations

Stefano Facchini, Attila Juhász, Giuseppe Lodato

Spatially resolved observations of protoplanetary discs are revealing that their inner regions can be warped or broken from the outer disc. A few mechanisms are known to lead to su…

astro-ph.SR2017★ 13 cited

Mid-infrared interferometric variability of DG Tau: implications for the inner-disk structure

J. Varga, K. É. Gabányi, P. Ábrahám +12

Context. DG Tau is a low-mass pre-main sequence star, whose strongly accreting protoplanetary disk exhibits a so-far enigmatic behavior: its mid-infrared thermal emission is strong…

astro-ph.EP2017★ 45 cited

A Multi-Wavelength Analysis of Dust and Gas in the SR 24S Transition Disk

P. Pinilla, L. M. Pérez, S. Andrews +9

We present new Atacama Large Millimeter/sub-millimeter Array (ALMA) 1.3 mm continuum observations of the SR 24S transition disk with an angular resolution (12 au ra…

astro-ph.EP2016★ 64 cited

ALMA reveals the anatomy of the mm-sized dust and molecular gas in the HD 97048 disk

Catherine Walsh, Attila Juhász, Gwendolyn Meeus +5

Transitional disks show a lack of excess emission at infrared wavelengths due to a large dust cavity, that is often corroborated by spatially resolved observations at ~ mm waveleng…