activity
20172026
most citedProperties of Hi-GAL clumps in the inner Galaxy]{The Hi-GAL compact source catalogue. I. The physical properties of the clumps in the inner Galaxy ()

201 citations · 433 across the 25 of their papers we have counts for

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Showing 2023Show all

5 papers · 1 filter

astro-ph.SR202320 cited

Brightness and mass accretion rate evolution during the 2022 burst of EX~Lupi

F. Cruz-Sáenz de Miera, Á. Kóspál, P. Ábrahám +18

EX Lupi is the prototype by which EXor-type outbursts were defined. It has experienced multiple accretion-related bursts and outbursts throughout the last decades, whose study have…

astro-ph.SR202314 cited

Gaia21bty: An EXor lightcurve exhibiting an FUor spectrum

Michał Siwak, Lynne A. Hillenbrand, Ágnes Kóspál +16

Gaia21bty, a pre-main sequence star that previously had shown aperiodic dips in its light curve, underwent a considerable mag brightening that occurred over a few mo…

astro-ph.SR2023

The Radial Distribution and Excitation of H2 around Young Stars in the HST-ULLYSES Survey

Kevin France, Nicole Arulanantham, Erin Maloney +8

The spatial distribution and evolution of gas in the inner 10 au of protoplanetary disks form the basis for estimating the initial conditions of planet formation. Among the most im…

astro-ph.SR2023

The Gaia alerted fading of the FUor-type star Gaia21elv

Zsófia Nagy, Sunkyung Park, Péter Ábrahám +26

FU Orionis objects (FUors) are eruptive young stars, which exhibit outbursts that last from decades to a century. Due to the duration of their outbursts, and to the fact that only…

astro-ph.SR2023

PENELLOPE IV. A comparison between optical forbidden lines and UV lines in the Orion OB1b and -Ori associations

M. Gangi, B. Nisini, C. F. Manara +17

Observing the spatial distribution and excitation processes of atomic and molecular gas in the inner regions (< 20 au) of young (< 10 Myr) protoplanetary disks helps us to understa…