Results 81 to 90 of about 539 (174)
Editorial: White Dwarfs in the Age of the Great Collaborations
Alejandro Hugo Córsico +6 more
doaj +1 more source
Dynamics of Large-Scale Solar Flows. [PDF]
Hotta H +4 more
europepmc +1 more source
Observational asteroseismology
A Dissertation Presented to the Faculty of Science at the University of Aarhus in Partial Fulfillment of the Requirements for the Degree of Doctor of ...
openaire +2 more sources
Editorial: Challenges of asteroseismology in the era of space missions
Javier Pascual-Granado +3 more
doaj +1 more source
Not all nitrogen-rich field stars originate from globular clusters
Globular clusters (GCs) are important tracers of the early Galactic assembly process, with some of their stars showing distinct chemical abundance patterns.
Leitinger E. I. +9 more
doaj +1 more source
Gravitational-wave asteroseismology with fundamental modes from compact binary inspirals. [PDF]
Pratten G, Schmidt P, Hinderer T.
europepmc +1 more source
Optimising the global detection of solar-like oscillations
Context. A well-established method exists for predicting the detectability of solar-like oscillations that has seen extensive application supporting target selection strategies for space-based photometric missions.
Lund Mikkel N., Chaplin William J.
doaj +1 more source
Near-critical magnetic fields in Kepler red giants
Context. The recent seismic detection of magnetic fields in the cores of red giants has provided the opportunity to characterize these fields, potentially allowing access to information about their origin and their role in the internal transport of ...
Deheuvels S. +4 more
doaj +1 more source
The intermediate neutron capture process
Context. The intermediate neutron-capture process (i-process) can occur during proton ingestion events (PIEs), which may take place in the early evolutionary phases of asymptotic giant branch (AGB) stars. Aims. We investigate the impact of rotational and
Choplin A. +4 more
doaj +1 more source
Asteroseismology is widely used for the precise mass determination of solar-like oscillating stars, based on individual frequency modeling or homological scaling relations.
Beck P. G. +13 more
doaj +1 more source

