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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

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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.SR2016★ 32 cited

New debris disks in nearby young moving groups

A. Moór, Á. Kóspál, P. Ábrahám +5

A significant fraction of nearby young moving group members harbor circumstellar debris dust disks. Due to their proximity and youth, these disks are attractive targets for studyin…

astro-ph.SR2015★ 96 cited

An M-dwarf star in the transition disk of Herbig HD 142527; Physical parameters and orbital elements

S. Lacour, B. Biller, A. Cheetham +29

HD 142527A is one of the most studied Herbig Ae/Be stars with a transitional disk, as it has the largest imaged gap in any protoplanetary disk: the gas is cleared from 30 to 90 AU.…

astro-ph.SR2015★ 1 cited

Discovery of molecular gas around HD 131835 in an APEX molecular line survey of bright debris disks

A. Moór, Th. Henning, A. Juhász +11

Debris disks are considered to be gas-poor, but recent observations revealed molecular or atomic gas in several 10-40 Myr old systems. We used the APEX and IRAM 30m radiotelescopes…