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20202026
most citedTime-dependent, long-term hydrodynamic simulations of the inner protoplanetary disk I: The importance of stellar magnetic torques

17 citations · 78 across the 13 of their papers we have counts for

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10 papers · 1 filter

astro-ph.SR2026

Preparing for the Early eVolution Explorer: Photometric Diagnostics of Magnetospheric Accretion Geometry in Young Stellar Objects

Laura Venuti, Connor E. Robinson, Ann Marie Cody +13

The inner disk truncation radius, , plays a crucial role in the regulation of star-disk interaction and the early evolution of star-disk-planet systems; however, measuring thi…

astro-ph.SR2026

The effect of variable stellar magnetic fields on the spin state of T Tauri stars

Lukas Gehrig, Daniel Steiner

Understanding the stellar spin evolution of young stars is crucial for understanding the evolution of protoplanetary disks and, consequently, the formation of exoplanets. According…

astro-ph.SR2025★ 4 cited

Protoplanetary disks around magnetized young stars with large-scale magnetic fields I: Steady-state solutions

D. Steiner, L. Gehrig, M. Güdel

Describing the large-scale field topology of protoplanetary disks faces significant difficulties and uncertainties. The transport of the large-scale field inside the disk plays an…

astro-ph.SR2025★ 2 cited

Do accretion-powered stellar winds help spin down T Tauri stars?

Lukas Gehrig, Eric Gaidos, Laura Venuti +2

How T Tauri stars remain slowly rotating while still accreting material is a long-standing puzzle. Current models suggest that these stars may lose angular momentum through magneto…

astro-ph.SR2023★ 4 cited

The post-disk (or primordial) spin distribution of M dwarf stars

L. Gehrig, E. Gaidos, M. Güdel

We investigate the influence of an accretion disk on the angular momentum (AM) evolution of young M dwarfs, which parameters govern the AM distribution after the disk phase, and wh…

astro-ph.SR2023★ 7 cited

What governs the spin distribution of very young < 1 Myr low mass stars

L. Gehrig, E. I. Vorobyov

We compute the evolution and rotational periods of young stars, using the MESA code, starting from a stellar seed, and take protostellar accretion, stellar winds, and the magnetic…

astro-ph.SR2022★ 11 cited

The influence of metallicity on a combined stellar and disk evolution

L. Gehrig, T. Steindl, E. I. Vorobyov +2

The effects of an accretion disk are crucial to understanding the evolution of young stars. During the combined evolution, stellar and disk parameters influence each other, motivat…

astro-ph.SR2022★ 14 cited

Time-dependent, long-term hydrodynamic simulations of the inner protoplanetary disk II: The importance of stellar rotation

Lukas Gehrig, Daniel Steiner, Eduard Vorobyov +1

The spin evolution of young protostars, surrounded by an accretion disk, still poses problems for observations and theoretical models. In recent studies, the importance of the magn…

astro-ph.SR2021★ 17 cited

Time-dependent, long-term hydrodynamic simulations of the inner protoplanetary disk I: The importance of stellar magnetic torques

D. Steiner, L. Gehrig, B. W. Ratschiner +4

We conduct simulations of the inner regions of protoplanetary disks (PPDs) to investigate the effects of protostellar magnetic fields on their long-term evolution. We use an inner…

astro-ph.SR2020

Mass limits for stationary protoplanetary accretion disks

Florian Ragossnig, Lukas Gehrig, Ernst A. Dorfi +2

The collapse of interstellar gaseous clouds towards a protostar leads to the formation of accretion disks around the central star. Such disks can be dynamically stable if they sett…