activity
20062021
most citedDetection of the Water Reservoir in a Forming Planetary System

305 citations · 2.3k across the 36 of their papers we have counts for

collaborators

36 papers

astro-ph.SR2021

Episodic accretion in focus: revealing the environment of FU Orionis-type stars

O. Fehér, Á. Kóspál, P. Ábrahám +3

The earliest phases of star formation are characterised by intense mass accretion from the circumstellar disk to the central star. One group of young stellar objects, the FU Orioni…

astro-ph.EP2020★ 79 cited

Global Hydromagnetic Simulations of Protoplanetary Disks with Stellar Irradiation and Simplified Thermochemistry

Oliver Gressel, Jon P. Ramsey, Christian Brinch +3

Outflows driven by large-scale magnetic fields likely play an important role in the evolution and dispersal of protoplanetary disks, and in setting the conditions for planet format…

astro-ph.SR2019★ 32 cited

Organic complexity in protostellar disk candidates

Jennifer B. Bergner, Rafael Martin-Domenech, Karin I. Oberg +3

We present ALMA observations of organic molecules towards five low-mass Class 0/I protostellar disk candidates in the Serpens cluster. Three sources (Ser-emb 1, Ser-emb 8, and Ser-…

astro-ph.SR2018★ 30 cited

Chemistry of a newly detected circumbinary disk in Ophiuchus

E. Artur de la Villarmois, L. E. Kristensen, J. K. Jørgensen +6

(Abridged) Astronomers recently started discovering exoplanets around binary systems. Therefore, understanding the formation and evolution of circumbinary disks is crucial for a co…

astro-ph.SR2017★ 55 cited

The ALMA-PILS survey: 3D modeling of the envelope, disks and dust filament of IRAS 16293-2422

S. K. Jacobsen, J. K. Jørgensen, M. H. D. van der Wiel +8

Context. The Class 0 protostellar binary IRAS 16293-2422 is an interesting target for (sub)millimeter observations due to, both, the rich chemistry toward the two main components o…

astro-ph.SR2017★ 23 cited

Interferometric view of the circumstellar envelopes of northern FU Orionis-type stars

O. Fehér, Á. Kóspál, P. Ábrahám +2

FU Orionis-type objects are young, low-mass stars with large outbursts in visible light that last for several years or decades. They are thought to represent an evolutionary phase…