Results 71 to 80 of about 37,244 (118)

SPINAL DISORDERS IN PROFESSIONAL ESPORTS ATHLETES: PROTOCOL FOR A SYSTEMATIC REVIEW. [PDF]

Acta Ortop Bras
Miachiro NY, de Menezes MD, Pontes MDS, Herrero CFPDS.   +3 more
europepmc   +1 more source

The emergence of globular clusters and globular-cluster-like dwarfs. [PDF]

Nature
Taylor ED, Read JI, Orkney MDA, Kim SY, Pontzen A, Agertz O, Rey MP, Andersson EP, Collins MLM, Yates RM.   +9 more
europepmc   +1 more source

The nucleardatapy toolkit for simple access to experimental nuclear data, astrophysical observations, and theoretical predictions. [PDF]

Eur Phys J A Hadron Nucl
Margueron J, Drischler C, Dutra M, Gandolfi S, Gezerlis A, Grams G, Guillot S, Kumar R, Lalit S, Lourenço O, Somasundaram R, Tews I, Vidaña I.   +12 more
europepmc   +1 more source

BMI, race and AF recurrence post ablation: a meta-analysis and systematic review. [PDF]

Front Cardiovasc Med
Xuejiao Y, Qianyu L, Xinzheng H, Yanfei L, Lanlan L, Yingtian Y, Chenyan Y, Manshi W, Yushan L, Xing C, Qian W, Shihan W.   +11 more
europepmc   +1 more source

Feasibility of longitudinal relaxation rate mapping with non-Cartesian sampling and compressed sensing on a 1.5 T magnetic resonance linear accelerator. [PDF]

Phys Imaging Radiat Oncol
McCullum L, van Rijssel MJ, Hwang KP, Ding Y, Tang C, Hassanzadeh C, Yang J, Balter PA, Wang J, Fuller CD, Subashi ED.   +10 more
europepmc   +1 more source

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Searching for Low Mass Stars in the Halo

Astrophysics and Space Science, 1999
From microlensing events detected at high galactic latitude as well as from direct measurements of the halo stellar density, estimations of a potential contribution of low mass stars to the mass budget is questioned. Up to now no clear answer has been found for one main reason: the difficulty to observe them in a sufficient volume, which requires deep ...
A.C. Robin, M. Crézé, V. Mohan
openaire   +1 more source

Very Low Mass Stars

Annual Review of Astronomy and Astrophysics, 1987
Very low mass (VLM) stars, which we define here somewhat arbitrarily as those with masses ;$ 0.3 M 0' pose some of the more interesting problems in stellar astrophysics. The physics of their envelopes and atmospheres are more complicated and their structures less well modeled than their more massive counterparts.
James Liebert, Ronald G. Probst
openaire   +2 more sources

Low mass stars

Astrophysics and Space Science, 1994
Low mass stars contribute an important fraction to the mass of our Galaxy. Due to the faintness of these stars a direct investigation of their space distribution and kinematics can be carried out only in the immediate solar neighbourhood. This fact emphasizes the importance of the “Third Catalogue of Nearby Stars” (CNS3) as a probe of the stellar ...
openaire   +1 more source