Results 211 to 220 of about 75,652 (263)
ABSTRACT Objective To determine whether myelin‐sensitive quantitative MRI reveals microstructural abnormalities in normal‐appearing cortex (NACtx) in myelin oligodendrocyte glycoprotein antibody–associated disease (MOGAD), indicating that conventional MRI underestimates remission residual cortical injury.
Valentina Camera +20 more
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Clonal Expansion of <i>penA</i>-60.001 in Cephalosporin-Resistant <i>Neisseria gonorrhoeae</i>: A Molecular Epidemiology Study in Meizhou, China, 2020-2024. [PDF]
Li Q +5 more
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<i>Neisseria gonorrhoeae</i> LIN codes provide a robust, multi-resolution lineage nomenclature. [PDF]
Unitt A +5 more
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Subcuticular symbionts of intertidal brittle stars: diversity, host specificity, and functional potential. [PDF]
Kawano K +5 more
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Dispersal Beyond Mountains and Borders: Asymmetrical Gene Flow Helps Maintain Brown Bear Metapopulation Connectivity on the Balkan Peninsula. [PDF]
Pylidis C +12 more
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Protocol for rapid allelic discrimination qPCR genotyping of the Winnie mouse model. [PDF]
Mansoori B, Liang C.
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The emergence of globular clusters and globular-cluster-like dwarfs. [PDF]
Taylor ED +9 more
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Proceedings of the thirteenth annual symposium on Computational geometry - SCG '97, 1997
We solve two open problems posed by Goodman and Pollack[GP84] about sets of signed circular permutations (clusters of stars) arising from generalized configurations of points: recognition and efficient reconstruction (drawing). As a biproduct we get an O(n2) space data structure constructible in O(n2) time, representing the order type of a (generalized)
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We solve two open problems posed by Goodman and Pollack[GP84] about sets of signed circular permutations (clusters of stars) arising from generalized configurations of points: recognition and efficient reconstruction (drawing). As a biproduct we get an O(n2) space data structure constructible in O(n2) time, representing the order type of a (generalized)
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1982
Astronomy and Astrophysics were first treated in volume III of the 6th edition of Landolt-Bornstein in 1952, then in volumes VI/1 and VI/2 of the New Series, 1965 and 1981/82 respectively. The present volume VI/3 is a further supplementation of volume VI/1.
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Astronomy and Astrophysics were first treated in volume III of the 6th edition of Landolt-Bornstein in 1952, then in volumes VI/1 and VI/2 of the New Series, 1965 and 1981/82 respectively. The present volume VI/3 is a further supplementation of volume VI/1.
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Understanding Stars and Star Clusters
2010Stars are formed from gas and dust compressed together by various forces. Star clusters are formed in several different ways. In what are called open clusters, it is usually the sweeping wave action of the spiral arms of the galaxy thrusting vast stretches of this interstellar material away from the galaxy.
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