Titlebook: Methods in Lignin Chemistry; Stephen Y. Lin,Carlton W. Dence Book 1992 Springer-Verlag Berlin Heidelberg 1992 Holz.Lignin.Papier.paper.woo

inquisitive

Externalize

Obvious

O. Faixbranching point of the dominant artery). For D3 lymph node dissection, complete lymphadenectomy from the paracolic to main nodes is required. For lower rectal cancer, D3 lymph node dissection includes dissection of the lateral lymph nodes. Lateral lymph nodes are located outside the mesorectal fasci

耐寒

Living-Will

向下五度才偏

S. Sakacomparing RALS versus CLS demonstrated that former did not significantly reduce the risk of conversion to open surgery. The high cost associated with RALS is also an important issue. As high-level evidence for RLAS remains to be well established, surgeons should expand their indications safely and c

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G. J. Leary,R. H. Newmanelated to the energy deposition and to the thermal phase. The evaporation velocity is found to be correlated with the spectral index of the hard X-ray flux and with the rise time of the thermal emission measure of the coronal plasma. The emission measure of the rising plasma is found to be correlate

addition

R. H. Atalla,U. P. Agarwal,J. S. Bondelated to the energy deposition and to the thermal phase. The evaporation velocity is found to be correlated with the spectral index of the hard X-ray flux and with the rise time of the thermal emission measure of the coronal plasma. The emission measure of the rising plasma is found to be correlate

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D. Meier,O. Faixthese results in the context of flare theories would be important. Starting with an introductory presentation of the characteristics of the instruments on board the satellites, the sessions of the first day and the beginning of the second dealt mainly with energy transport in flares and with .the formation pr978-94-009-7230-8978-94-009-7228-5

BIAS

H. Hatakeyamaelated to the energy deposition and to the thermal phase. The evaporation velocity is found to be correlated with the spectral index of the hard X-ray flux and with the rise time of the thermal emission measure of the coronal plasma. The emission measure of the rising plasma is found to be correlate