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We evaluated the prognostic relevance of impaired glucose metabolism (IGM) in a cohort of patients with Stage I breast cancer, with no need for systemic adjuvant treatment. The cohort included 955 patients surgically treated for Stage I breast cancer in a single institution between 1988 and 2007. Each patient had glucose metabolism evaluated by oral glucose tolerance test (OGTT) after a mean of 4.4 +/- 2.8 years. Patients with known diabetes were excluded. During a median follow-up period of 22.1 years, 295 women developed recurrent disease and 186 died. When age and pathological tumor size were adjusted, the hazard ratios (HRs) for recurrence and death were 1.16 (95% confidence interval, 0.97-1.38; P =.109) and 1.17 (95% confidence interval, 0.97-1.41; P =.097), respectively, for women with vs women without IGM. However, in patients without receiving chemotherapy, the risks of recurrence and death were significantly higher (HRs = 1.35 and 1.61, respectively; P =.012 and P
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In a paper published today in the Astrophysical Journal, a team of scientists examined data collected by the Helioseismic and Magnetic Imager (HMI) instrument on NASA’s Solar Dynamics Observatory.
“The best data we’ve seen to date show a dipole magnetic field with an uneven distribution, which is different from what we’d expect to see in a regular, solar cycle,” said researcher Elinor Roy of the University of Hawaii, lead author of the paper. “The uniformity of the magnetic field suggests that there are more ‘attractor’ regions in the solar corona.”
The solar corona is a part of the sun’s atmosphere, extending to 10 million miles (15 million kilometers) in Earth’s direction above the sun’s surface. The solar corona and the sun’s magnetic field protect the sun’s atmosphere from particles streaming out from the sun’s surface.
HMI’s observations show that the magnetic field is not uniform at the surface, but rather a mixture of areas of strong and weak magnetic fields.
“We see where the field is weaker, where the magnetism is weaker, and where it is stronger in the corona,” Roy said. “This appears to be an artefact of the turbulence in the solar corona that we have not been able to reduce and model. We will continue to refine our analysis of HMI and
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Current pharmacological therapies for obstructive sleep apnea–hypopnea syndrome (OSAHS) that are targeted to the central nervous system are not fully effective and are associated with significant adverse effects. Considering the rapidly growing number of adults with OSAHS and at an increased risk for chronic disease, it is clear that developing new therapies and targeting them specifically to the site of action is prudent. Preclinical studies in multiple animal models of sleep disordered breathing are providing important insights into the pathophysiology of OSAHS and identifying potential therapeutic targets in the brain that are associated with more normal and effective sleep, including cognitive performance. Neuromodulators such as adenosine, orexin, and opioids may represent a novel therapeutic approach for patients with OSAHS.
In this article, the authors review evidence supporting the use of neuromodulators and stimulants as treatment options for OSAHS.
We searched Medline for relevant articles that were published between 1966 and July 2006. The terms “sleep,” “adenosine,” “caffeine,” “opiates,” and “ghrelin” were combined with the key terms “obstructive sleep apnea/hypopnea syndrome,” “monotherapy,” “decreased sleep efficiency,” “hypoxemia,” “headache,” and “adverse events.” Other potentially relevant studies from the reference lists of these articles were also considered.
This review covers four important aspects of OSAHS: (1) anatomy and physiology of the brain and mechanisms underlying OSAHS; (2) recent advances in preclinical studies that shed light
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AMS Software Home Photo Studio v2.71 with SERIAL setup free
AMS Software Home Photo Studio v2.71 with SERIAL setup free
AMS Software Home Photo Studio v2.71 with SERIAL setup free
AMS Software Home Photo Studio v2.71 with SERIAL setup free
You must back up important files, data, photos, videos, etc. before you try to install an AMS system. Without Windows. For more information about the AMS Software logo and the.Semen storferi
Semen storferi is a rare species of grass known by the common name Castle Mountain caltrop. It is native to the southwestern United States and northern Mexico, where it grows in sagebrush and creosote bush and other desert scrub habitat.
Description
Semen storferi is an annual grass growing up to around 20 centimeters in maximum height. The linear to lance-shaped leaves are borne in a basal rosette, each no more than 4.5 centimeters long.
The inflorescence is a single cymose cluster of several spikelets each a few millimeters long. The clusters have a total of 10-25 spikelets per cluster. Each spikelet has two to three flowers.
References
External links
Jepson Manual Treatment
USDA Plants Profile
Grass Manual Treatment
storferi
Category:Native grasses of California
Category:Grasses of Mexico
Category:Grasses of the United States
Category:Flora of the Southwestern United States
Category:Flora of the South-Central United States
Category:Flora of the California desert regions
Category:Flora of Northwestern Mexico issues.
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