Results 1 to 10 of about 98,425 (396)
Technetium Complexes with 1,1-Dicyanoethene-2,2-diselenolate,i-mns2-. The Crystal Structure of (Bu4N)2[TcN(i-mns)2] [PDF]
Ulrich Abram +4 more
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The Nuclear Imaging Uncertainty Principle. Do Nuclear Cameras Really Work? [PDF]
The introduction of the Heisenberg Uncertainty principle and Nuclear Cardiology occurred simultaneously in 1925-1927. Thirty years later the Anger gamma camera would allow for a more sophisticated radioactive isotope counting to determine the presence or
Gordon Harrington, Richard Fleming
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Extracardiac Accumulation of Technetium-99m-Pyrophosphate in Transthyretin Cardiac Amyloidosis
Koji Takahashi +9 more
openalex +1 more source
The role of 99mTc-Ubiquicidin (UBI) and 99mTc-IgG scintigraphies in diagnosis of acute appendicitis: A preliminary result [PDF]
Introduction: Appendicitis is one of the most common surgical emergencies. In spite of the relatively high rate of negative appendectomy, as a result of miss diagnosis, uncertainty of diagnosis still continues to challenge physicians.
Assadi, M. +6 more
core
During the evolution on the AGB, S-type stars are the first objects to experience s-process nucleosynthesis and third dredge-ups, and therefore to exhibit sprocess signatures in their atmospheres. Their significant mass loss rates (10^-7 to 10^-6 M*/year)
Goriely, Stéphane +5 more
core
Nuclear medicine: investigation of renal function in small animal medicine [PDF]
Kidney function investigations in veterinary medicine are traditionally based on blood analysis (blood urea nitrogen (BUN) and serum creatinine concentration) and / or urinalysis (urine specific gravity, protein-to-creatinine ratio or fractional ...
De Sadeleer, Carlos +7 more
core
Context- S stars are late-type giants with spectra showing characteristic molecular bands of ZrO in addition to the TiO bands typical of M stars. Their overabundance pattern shows the signature of s-process nucleosynthesis.
Goriely, Stephane +5 more
core +1 more source

