31 citations · 148 across the 11 of their papers we have counts for
11 papers
Solar-like oscillations in accreting pre-main sequence stars: Insights and prospects
Johannes Jørgensen, Konstanze Zwintz, Ebraheem Farag +2
We present theoretical predictions for solar-like oscillators in the pre-main sequence phase of stellar evolution. Our pre-main sequence models start from a stellar seed of 0.01 so…
Catalogue of BRITE-Constellation targets I. Fields 1 to 14 (November 2013 - April 2016)
K. Zwintz, A. Pigulski, R. Kuschnig +25
The BRIght Target Explorer (BRITE) mission collects photometric time series in two passbands aiming to investigate stellar structure and evolution. Since their launches in the year…
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…
The imprint of star formation on stellar pulsations
Thomas Steindl, Konstanze Zwintz, Eduard Vorobyov
In the earliest phases of their evolution, stars gain mass through the acquisition of matter from their birth clouds. The widely accepted classical concept of early stellar evoluti…
The Pre-main Sequence: Challenges and Prospects for Asteroseismology
Konstanze Zwintz, Thomas Steindl
Stars do not simply pop up on the main sequence. Before the stars arrive on the zero-age main sequence, they form in the collapses of molecular clouds, gain matter through accretio…
Pulsational instability of pre-main-sequence models from accreting protostars II. Modelling echelle diagrams of Scuti stars without rotational splitting
T. Steindl, K. Zwintz, M. Müllner
The physics of early stellar evolution (e.g. accretion processes) is often not properly included in the calculations of pre-main-sequence models, leading to insufficient model grid…