Results 211 to 220 of about 1,914,471 (252)
Nanoscale geometrical patterning for junctionless thermoelectrics
Gonzalez-Munoz S +12 more
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Ophthalmology Clinics of North America, 2002
Spontaneous closure of macular holes occurs in 3% to 9% of patients over 6 years [3,58]. Visual acuity can recover dramatically once the hole closes. The risk for hole development in the fellow eye in the absence of PVD is approximately 29%. The presence of vitreomacular separation reduces the risk to less than 5%.
Michael, Landolfi +2 more
openaire +2 more sources
Spontaneous closure of macular holes occurs in 3% to 9% of patients over 6 years [3,58]. Visual acuity can recover dramatically once the hole closes. The risk for hole development in the fellow eye in the absence of PVD is approximately 29%. The presence of vitreomacular separation reduces the risk to less than 5%.
Michael, Landolfi +2 more
openaire +2 more sources
Albrecht von Graefe's Archive for Clinical and Experimental Ophthalmology, 1980
Twenty-four eyes with macular holes have been followed for periods ranging from one to four years. Each hole was demonstrated, clinically, to be full thickness and associated with a small, localized, retinal detachment and a posterior vitreous separation.
M, James, S S, Feman
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Twenty-four eyes with macular holes have been followed for periods ranging from one to four years. Each hole was demonstrated, clinically, to be full thickness and associated with a small, localized, retinal detachment and a posterior vitreous separation.
M, James, S S, Feman
openaire +2 more sources
Advances in Health Sciences Education
In this editorial the editor looks into holes in scholarship in the field of health professions education and their implications for understanding and developing the field.
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In this editorial the editor looks into holes in scholarship in the field of health professions education and their implications for understanding and developing the field.
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2009
Abstract A black hole is an object that is inside its event horizon at r=r*: a one-way surface that particles and light can only traverse inward. This chapter studies the spherically symmetric nonrotating Schwarzschild black hole. The metric elements change their respective signs when crossing from r>r∗ to r<r*, leading to ...
openaire +1 more source
Abstract A black hole is an object that is inside its event horizon at r=r*: a one-way surface that particles and light can only traverse inward. This chapter studies the spherically symmetric nonrotating Schwarzschild black hole. The metric elements change their respective signs when crossing from r>r∗ to r<r*, leading to ...
openaire +1 more source