Results 81 to 90 of about 461 (261)

Toward a Comprehensive Grid of Cepheid Models with MESA. IV. Modest Effects of Rotation on Blue Loops

open access: yesThe Astrophysical Journal Supplement Series
Evolutionary tracks for 2–8 M _⊙ stars, with metallicities of Z = 0.014, 0.006, and 0.002, including rotation, are computed with Modules for Experiments in Stellar Astrophysics ( MESA ).
Radoslaw Smolec   +2 more
doaj   +1 more source

Excitation of stellar pulsations

open access: yes, 2011
Invited paper to be published in: Proc. 61st Fujihara Seminar "Progress in solar/stellar physics with helio- and asteroseismology", Shibahashi H., ed., Hakone, 12 pages, 6 ...
openaire   +2 more sources

The Role of Opacities in Stellar Pulsation

open access: yes, 2018
6 pages, 3 Figures, Proceeding for the "Workshop on Astrophysical Opacities"
Kanbur, S. M.   +4 more
openaire   +3 more sources

Low‐Angle Grain Boundaries and Re‐Segregation in Single‐Crystalline Ni‐Base Superalloys

open access: yesAdvanced Engineering Materials, EarlyView.
This work demonstrates that Re‐segregation at low‐angle grain boundaries (LAGBs) in Ni‐base superalloys is influenced by misorientation angle. Advanced microscopy and atom probe tomography reveal that higher misorientation angles increases Re‐segregation.
Alireza B. Parsa   +9 more
wiley   +1 more source

Time‐Dependent Oxidation and Scale Evolution of a Wrought Co/Ni‐Based Superalloy

open access: yesAdvanced Engineering Materials, EarlyView.
This study shows how a new wrought Co/Ni‐based superalloy resists oxidation at 800 ∘$^\circ$C. The oxide scale changes from rough, fast‐growing spinel to a dense, protective chromia–alumina layer. Atom probe analysis reveals tiny refractory‐rich bubbles at the interface that mark the transition to long‐term, diffusion‐controlled protection ...
Cameron Crabb   +6 more
wiley   +1 more source

The Asteroseismological Richness of RCB and dLHdC Stars

open access: yesThe Astrophysical Journal
RCB stars are L ≈ 10 ^4 L _⊙ solar-mass objects that can exhibit large periods of extinction from dust ejection episodes. Many exhibit semi-regular pulsations in the range of 30–50 days with semi-amplitudes of 0.05–0.3 mag.
Tin Long Sunny Wong, Lars Bildsten
doaj   +1 more source

Slip Localization Intensification Mediated by Grain Boundary Sliding in a Polycrystalline Nickel‐Based Superalloy

open access: yesAdvanced Engineering Materials, EarlyView.
The temperature dependence of fatigue behavior in nickel‐based superalloys is investigated through high‐resolution measurements of plastic localization. While increasing temperature reduces localization and enhances fatigue performance in René 88DT, Inconel 718 exhibits a sharp degradation at intermediate temperature due to intensified slip ...
M. Calvat   +5 more
wiley   +1 more source

Pulsational Mass Loss from Supermassive Stars Creates the Compact Shells of Little Red Dots

open access: yesThe Astrophysical Journal Letters
Little Red Dots (LRDs) have emerged as one of the central puzzles of the JWST era. Their spectra increasingly require dense gas close to the source, yet the physical origin of that cocoon-like structure remains unclear.
Devesh Nandal   +5 more
doaj   +1 more source

Fatigue Crack Initiation and Growth in Nanocrystalline Ni at Multiple Length‐Scales

open access: yesAdvanced Engineering Materials, EarlyView.
Overview of miniaturized in situ SEM fatigue setup and resultant fatigue crack growth data for nanocrystalline Ni. The presented study focuses on the analysis of fatigue crack growth rate (FCGR) in focused ion beam‐notched microcantilevers prepared from nanocrystalline (NC) Ni as a model material.
Igor Moravcik   +7 more
wiley   +1 more source

Stellar Atmospheric Parameters of ∼11,000 RR Lyrae Stars from LAMOST Spectra

open access: yesThe Astrophysical Journal Supplement Series
Accurate determination of the stellar atmospheric parameters of RR Lyrae stars (RRLs) requires short individual exposures of the spectra to mitigate pulsation effects.
Jiangtao Wang   +4 more
doaj   +1 more source

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