Nagoya University

About: Nagoya University is a education organization based out in Nagoya, Japan. It is known for research contribution in the topics: Population & Catalysis. The organization has 58009 authors who have published 128227 publications receiving 3246340 citations. The organization is also known as: Nagoya Daigaku & Meidai.

Revision of diagnostic guidelines for Kawasaki disease (the 5th revised edition).

Abstract: Diagnostic guidelines for Kawasaki Disease was revised to meet the present situation in 2002. This issue intends to explain new guidelines and their backgrounds. Major alterations are interpretation of cases with 4 or fewer febrile days shortened by early intravenous immunoglobulin treatment, and the clinical importance of atypical (incomplete, or suspected) cases.

Hepatic segmentectomy with caudate lobe resection for bile duct carcinoma of the hepatic hilus.

Abstract: From 1979 through 1989, surgical resection was performed in 55 of 66 patients with carcinoma of the hepatic hilus after improving jaundice by percutaneous transhepatic biliary drainage (PTBD). Selective cholangiography through PTBD was done to define precisely the anatomical location--extent of the obstructing lesion in each segmental hepatic duct. Percutaneous transhepatic cholangioscopy was performed through the sinus tract of PTBD after replacing the drainage catheter with a 15 French catheter for superselective cholangiography and biopsy to make the definitive diagnosis of the histological extent of the tumor and any variation of each segmental hepatic duct that joins the hepatic hilus. In 46 (69.7%) of 66 patients, curative resection was possible. Forty-five of these underwent various types of hepatic segmentectomy with caudate lobectomy for a morbidity rate of 41.3% and an operative mortality rate of 6.4%. Fourteen (31.1%) advanced cases underwent combined resection of the portal vein together with hepatectomy. Microscopic tumor involvement in the caudate branches was confirmed in 44 of 45 patients who underwent caudate lobe resection. The 3-year survival rate for all 43 patients surviving the curative excision was 55.1% and the 5-year survival rate was 40.5%. All 11 patients who had an unresectable advanced tumor died within 9 months. Curative resection should be designed according to the preoperative findings of the extent of cancer in each segmental duct, and caudate lobe resection should be performed together with the smallest necessary hepatic segmentectomy possible.

Planck early results. XIX. All-sky temperature and dust optical depth from Planck and IRAS. Constraints on the "dark gas" in our Galaxy

Abstract: An all sky map of the apparent temperature and optical depth of thermal dust emission is constructed using the Planck-HFI (350μm to 2 mm) andIRAS(100μm) data. The optical depth maps are correlated with tracers of the atomic (Hi) and molecular gas traced by CO. The correlation with the column density of observed gas is linear in the lowest column density regions at high Galactic latitudes. At high N(H), the correlation is consistent with that of the lowest NH, for a given choice of the CO-to-H(2) conversion factor. In the intermediate NH range, a departure from linearity is observed, with the dust optical depth in excess of the correlation. This excess emission is attributed to thermal emission by dust associated with a dark gas phase, undetected in the available Hi and CO surveys. The 2D spatial distribution of the dark gas in the solar neighbourhood (|b(II)| > 10°) is shown to extend around known molecular regions traced by CO. The average dust emissivity in the Hi phase in the solar neighbourhood is found to be τ(D)/N(H)(tot) = 5.2×10(-26) cm(2) at 857 GHz. It follows roughly a power law distribution with a spectral index β = 1.8 all the way down to 3 mm, although the SED flattens slightly in the millimetre. Taking into account the spectral shape of the dust optical depth, the emissivity is consistent with previous values derived fromFIRAS measurements at high latitudes within 10%. The threshold for the existence of the dark gas is found at N(H)(tot) = (8.0±0.58)×10(20) H cm(−2) (A(V )= 0.4mag). Assuming the same high frequency emissivity for the dust in the atomic and the molecular phases leads to an average X(CO) = (2.54 ± 0.13) × 10(20) H(2) cm(-2)/(K km s(-1)). The mass of dark gas is found to be 28% of the atomic gas and 118% of the CO emitting gas in the solar neighbourhood. The Galactic latitude distribution shows that its mass fraction is relatively constant down to a few degrees from the Galactic plane. A possible explanation for the dark gas lies in a dark molecular phase, where H2 survives photodissociation but CO does not. The observed transition for the onsetof this phase in the solar neighbourhood (AV = 0.4mag) appears consistent with recent theoretical predictions. It is also possible that up to half of the dark gas could be in atomic form, due to optical depth effects in the Hi measurements.