Results 41 to 50 of about 10,274 (118)
Zams Rotational Velocities of be Stars
, 2005 We show that Be stars belong to a high velocity tail of a single B-type star rotational velocity distribution in the main sequence (MS). We studied 127 galactic field Be stars and obtained their true equatorial velocity at the ZAMS using models of stellar evolution with rotation.
Zorec, Juan +4 more
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Limiting rotational period of neutron stars [PDF]
Physical Review D, 1992 Pulsars have been identified with the theoretical objects called neutron stars. The identification is convincing—but not proved. The short rotational periods of millisecond pulsars inform us that the average density (and, therefore, the central density) must be very high—higher than the density of nuclei (5.8).
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On the Rotation of the Stars [PDF]
Monthly Notices of the Royal Astronomical Society, 1929 G. Shajn, O. Struve
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On the existence of ergoregions in rotating stars [PDF]
Monthly Notices of the Royal Astronomical Society, 1978 Schutz, B., Comins, N.
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Precision Enhancement of Multi-Source Integrated Navigation via Solar Disk Differential Velocity Compensation. [PDF]
Sensors (Basel)Huang Y, Ning X.
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Trifluoroacetylation and Sulfur Oxidation States Modulate Cis-Trans Isomerization and Atropisomerism in N-Aryl Peptoids. [PDF]
ChiralityRaju NKM +5 more
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B-type host stars revealed by exoplanets around massive secondary-clump giant stars. [PDF]
Nat CommunLin WX +14 more
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Development of a mobile application tracking stats and goals of young basketball players: design-based research. [PDF]
Front PsycholTascioglu R +3 more
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Machine learning-enabled membership determination of open cluster AH03_J0748-26.9 using Gaia DR3 astrometry. [PDF]
Sci RepBadawy WA, Abdel Rahman HI.
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