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pro vyhledávání: '"Richard J. Allison"'
British swimmers are at a heightened risk of vitamin D deficiency (serum 25-hydroxyvitamin D (25(OH)D): − 1) as their large indoor training volumes often restrict sunlight exposure, especially during the winter when daylight hours are reduced. Prev
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8222c5c2c2ef386be7144cdb2e50dcaf
https://doi.org/10.21203/rs.3.rs-1463196/v1
https://doi.org/10.21203/rs.3.rs-1463196/v1
Autor:
Graeme L. Close, Bruce A. Hamilton, Anissa Cherif, Mathew G Wilson, Richard J. Allison, Abdulaziz Farooq
Publikováno v:
British Journal of Sports Medicine. 52:522-526
BackgroundThe association between bone mineral density (BMD) and serum25-hydroxyvitamin D (25(OH)D) concentration is weak, particularly in certain races (eg, BlackAfrican vs Caucasian) and in athletic populations. We aimed to examine if bioavailable
Autor:
Richard J. Allison, Graeme L. Close, Abdulaziz Farooq, Bruce A. Hamilton, Mathew G Wilson, Nathan R Riding, Othman Salah
Publikováno v:
European Journal of Preventive Cardiology. 22:535-542
Vitamin D (25(OH)D) deficiency has associations with bowl/colon cancer, arthritis, diabetes, and cardiovascular disease. Many athletes are vitamin D deficient, yet no studies have examined the association between 25(OH)D status and cardiac structure
Autor:
Richard J. Allison
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 421:3338-3342
We investigate how the properties of escaping stars are related to the initial conditions of their birth clusters. We find that the number of escaping stars, their spatial distribution and their kinematics show a dependence on the initial conditions
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 418:2565-2575
Observations and theory suggest that star clusters can form in a subvirial (cool) state and are highly substructured. Such initial conditions have been proposed to explain the level of mass segregation in clusters through dynamics, and have also been
Autor:
Simon P. Goodwin, Richard J. Allison
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 415:1967-1976
We investigate the formation and evolution of high-order massive star multiples similar to the Trapezium in the Orion Nebula Cluster. We perform ensembles of N-body simulations of the evolution of N=1000 Orion-like clusters with initial conditions ra
Autor:
Manuel Güdel, Estelle Moraux, Richard J. Allison, Richard J. Parker, S. Guieu, Simon P. Goodwin, Jerome Bouvier
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 412:2489-2497
We use the new minimum spanning tree (MST) method to look for mass segregation inthe Taurus association. The method computes the ratio of MST lengths of any chosensubset of objects, including the most massive stars and brown dwarfs, to the MSTlengths
Autor:
Simon P. Goodwin, Richard J. Parker, Simon Portegies Zwart, Richard de Grijs, Richard J. Allison
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 407:1098-1107
Observations and theory both suggest that star clusters form sub-virial (cool) with highly sub-structured distributions. We perform a large ensemble of N-body simulations of moderate-sized (N=1000) cool, fractal clusters to investigate their early dy
Autor:
M. B. N. Kouwenhoven, Richard J. Allison, Richard de Grijs, Richard J. Parker, Simon Portegies Zwart, Simon P. Goodwin
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 395(3), 1449-1454. Oxford University Press
We present a new method to detect and quantify mass segregation in star clusters. It compares the minimum spanning tree (MST) of massive stars with that of random stars. If mass segregation is present, the MST length of the most massive stars will be
Publikováno v:
Medicine & Science in Sports & Exercise. 48:307-308