Results 171 to 180 of about 112,697 (340)
Constraining Stellar Rotation at the Zero-age Main Sequence with TESS
The zero-age main sequence (ZAMS) is a critical phase for stellar angular momentum evolution, as stars transition from contraction-dominated spin-up to magnetic wind-dominated spin-down.
S. T. Douglas+7 more
doaj +1 more source
Studies in Stellar Rotation. III. A Redertimination of Rotational Velocities in the Pleiades.
Christopher M. Anderson+2 more
openalex +2 more sources
New Radiation Driven Wind Solutions Including Stellar Rotation: Applicability to Be stars [PDF]
M. Curé
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The share of technical thermoplastics is expected to grow further in the e‐mobility segment. In this study, a detailed temperature‐based tribological characterization of technical thermoplastics is performed. The tribological properties are discussed in terms of the dynamic mechanical properties of polymers at different ambient temperatures. A proof of
Harsha Raghuram+2 more
wiley +1 more source
Primary phases and a fatigue crack are studied in a forged blank of an aluminum alloy using synchrotron and laboratory X‐ray computed tomography. To image the crack, the fatigue test is interrupted, and a static tensile load is applied to open the crack.
Jakob Schröder+6 more
wiley +1 more source
An Edge-on Regular Disk Galaxy at z = 5.289
While rotation-supported gas disks are known to exist as early as at z ≈ 7, it is still a general belief that stellar disks form late in the Universe.
Haojing Yan+2 more
doaj +1 more source
Rotation-induced lithium depletion of solar-type stars in open stellar clusters [PDF]
R. Tschäpe, G. Rüdiger
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Multilayering of TiN film with metallic Ti film is adopted to enhance the fracture resistance of TiN thin films. Plastic dissipation within Ti with process zone size of ≈250 nm, along with elastic–plastic mismatch driven changes to crack driving force enhances the crack growth resistance by ten times, enabling physics informed design of optimized ...
Nidhin George Mathews+5 more
wiley +1 more source
From Infall to Rotation around Young Stellar Objects: A Transitional Phase with a 2000 AU Radius Contracting Disk? [PDF]
M. R. Hogerheijde
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