نتایج جستجو برای: â â â aside from its annual and seasonal fluctuation
تعداد نتایج: 17657463 فیلتر نتایج به سال:
â â significance of taking notice of pronouns in the selected poems of âmahmoud darwishâ â â â â fatemeh lotfigoodarzi * â pabiyah bent alhaj maming ** â â abstract â â â eltifat is one of the most prominent artistic techniques that impressively drew the attention of the old and modern poets. this rhetorical style bestows richness to texts and contributes to avoiding direct addres...
Aims—To investigate the expression of â-catenin in non-small-cell lung cancer (NSCLC) and its clinical significance. Methods—101 patients were surgically treated for NSCLC by lobectomy or pneumectomy with systematic lymph node dissection. Follow up was available in all patients, ranging from 24 to 110 months. Immunostaining of tissue sections from primary tumours and (when present) their lymph ...
The 0-24-h urinary metabolic profile of cyclophosphamide was inves tigated in a series of 14 patients with various malignancies receiving combination chemotherapy including i.v. cyclophosphamide. This was accomplished using combined thin-layer chromatography-photographydensitometry, which can quantitate cyclophosphamide and its four prin cipal urinary metabolites (4-ketocyclophosphamide, nor-ni...
ß à á â ã ä å â ae ç è é ê ë ì é í ä ì î ã á â ï í ð ñ ò à á â ã ä å ó ô ñ ï ì í õ ã ä ä â ä ô ö ô ÷ î ã á â ï í ð ñ ø à á â ã ä å ó â ù ú ë í ì ÷ é ê ö ä ã ì ñ î ã á â ï í ð ñ
We derive an efficient CH-type inequality. Quantum mechanics violates our proposed inequality independent of the detection-efficiency problem. In photonic Bell-type experiments [1], when photon pairs with parallel linear polarizations are emitted, one can consider a Clauser-Horne (CH) inequality [2], at the level of hidden variables, in the form − 1 ≤ Srq,HV (â, b̂, â, b̂, λ) ≤ 0 (1) where Srq,HV...
The limited angular resolution of γ–ray telescopes prevents the straight identification of the majority of the sources detected so far. This is particularly true for the low latitude, probably galactic ones, only 10 % of which has been identified. Most of the counterparts are Isolated Neutron Stars, both radio–loud and radio–quiet, characterised by an extremely high value of fX /fopt. The best ...
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