M. Muellner

Pulsational instability of pre-main-sequence models from accreting protostars. I. Constraining the input physics for accretion with spectroscopic parameters and stellar pulsations

T. Barnes, T. Steindl, K. Zwintz, 2021, Astronomy & Astrophysics.

Revisiting the pulsational characteristics of the exoplanet host star β Pictoris

S. N. Mellon, T. Guillot, L. Abe, 2019, Astronomy & Astrophysics.

Cross sections for neutron-producing reactions induced by 14. 1 MeV neutrons incident on /sup 6/Li, /sup 7/Li, /sup 10/B, /sup 11/B, and carbon

D. Drake, P. Lisowski, M. Drosg, 1988 .

β Cas: The first δ Scuti star with a dynamo magnetic field

C. Neiner, G. Wade, G. Handler, 2020, Astronomy & Astrophysics.

An analysis of the sharpness of monotonicity results via homotopy for sequential fractional operators

Christopher S. Goodrich, Matthew Muellner, C. Goodrich, 2019, Appl. Math. Lett..