Results 221 to 230 of about 85,442 (265)

In Search of Ideal Analgesia: Classical and Deep Rectus Sheath Block in Laparoscopic Cholecystectomy. [PDF]

Local Reg Anesth
Chooklin S, Chuklin S.
europepmc   +1 more source

High-Value Care Inclusion in the Preclinical and Clinical Years of Medical School: A Narrative Review and Descriptive Experience at a Single Institution. [PDF]

Cureus
Storm LK, Salvemini JD, Shields ML, Harris SK, Roux JA, Couey CC, Yang J, Doherty CG, Overton JS, Jeter JB.   +9 more
europepmc   +1 more source

Caregiver burden, quality of life, and psychosocial outcomes among informal caregivers of patients with glioma: A systematic review and meta-analysis. [PDF]

Asia Pac J Oncol Nurs
Wei H, Zhang S, Tao S, Li J, Liu X.
europepmc   +1 more source

Wind variability in early-type stars

, 1993
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Early-type emission-line stars

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Emission-line Stars and Early-type Stars with Gaia [PDF]

EAS Publications Series, 2010
Gaia will provide accurate parallaxes, spectrophotometry and spectroscopy for hundreds of thousands of emission-line stars across the whole HR diagram. In preparation for the Gaia mission, we are developing algorithms to recognize and classify emission-line stars. A large collection of ground-based spectroscopic observations has been collected and will
R. Blomme, Y. Frémat, A. Lobel, C. Martayan   +3 more
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Magnetism in massive early-type stars [PDF]

EAS Publications Series, 2013
In the last five years our knowledge of magnetism in early-type stars has significantly improved because of the new gen- eration of high-resolution spectropolarimeters (ESPaDOnS@CFHT, Narval@TBL, HARPSpol@ESO). The success of the Magnetism in Massive Stars (MiMeS) Project, for example, has greatly improved our understanding of the magnetic properties ...
J.H. Grunhut, G.A. Wade
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Isophot Observations of Early-Type Stars

Astrophysics and Space Science, 1997
Mass loss has an important effect on the evolution of early-type stars. The most reliable mass loss rates are determined from the radio continuum. However there is a wealth of observational evidence (Discrete Absorption Components, X-rays, IR continuum, Hα variability, …) indicating that the stellar wind is clumped.
R. Blomme, M.C. Runacres, K. Vyverman, M. Cohen, C. Leitherer, S. P. Owocki, M. Haas   +6 more
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