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20032026
most citedNearby debris disk systems with high fractional luminosity reconsidered

223 citations · 1.6k across the 34 of their papers we have counts for

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astro-ph.SR2022★ 6 cited

Mid-infrared time-domain study of recent dust production events in the extreme debris disc of TYC 4209-1322-1

A. Moór, P. Ábrahám, Á. Kóspál +23

Extreme debris discs are characterized by unusually strong mid-infrared excess emission, which often proves to be variable. The warm dust in these discs is of transient nature and…

astro-ph.SR2022★ 9 cited

Accretion and extinction variations in the low-mass pre-main sequence binary system WX Cha

Eleonora Fiorellino, Gabriella Zsidi, Agnes Kospal +5

Light curves of young star systems show photometric variability due to different kinematic, and physical processes. One of the main contributors to the photometric variability is t…

astro-ph.SR2020★ 11 cited

Grain growth in newly discovered young eruptive stars

Á. Kóspál, P. Ábrahám, A. Carmona +4

FU Orionis-type stars are young stellar objects showing large outbursts due to highly enhanced accretion from the circumstellar disk onto the protostar. FUor-type outbursts happen…

astro-ph.SR2019★ 91 cited

Identification of Young Stellar Object candidates in the DR2 x AllWISE catalogue with machine learning methods

G. Marton, P. Ábrahám, E. Szegedi-Elek +8

The second Data Release (DR2) contains astrometric and photometric data for more than 1.6 billion objects with mean magnitude 20.7, including many Young Stella…

astro-ph.SR2019★ 10 cited

Dust evolution in the circumstellar disc of the unclassified B[e] star HD 50138

J. Varga, T. Gerják, P. Ábrahám +3

We studied the disc of the unclassified B[e] star HD 50138, in order to explore its structure, and to find indications for the evolutionary status of this system, whether it is a y…

astro-ph.SR2018★ 15 cited

The outbursting protostar 2MASS~22352345+7517076 and its environment

Maria Kun, Peter Abraham, Jose Antonio Acosta Pulido +2

We studied the Class I protostar 2MASS 22352345+7517076 whose dramatic brightening between the IRAS, Akari, and WISE surveys was reported by Onozato et al. (2015). 2MASS 22352345+7…