Clinical Features of Oral Multiple Primary Carcinomas Compared with Oral Single Primary Carcinoma

[Background] Owing to the increase in the older population and the increased life span, the number of patients with oral multiple primary carcinomas will increase. Predicting the second and third carcinoma clinically is difficult, and the presence of second or third carcinomas is a factor that determines the prognosis of oral carcinoma. In this study, we examined the clinical features of oral multiple primary carcinomas treated in our department. [Methods] We retrospectively reviewed the medical records of patients with oral squamous cell carcinoma who underwent radical treatment at and were followed by the Department of Oral and Maxillofacial Surgery, Tottori University Hospital from January 2003 to October 2017. [Results] This study included 261 patients: 241 patients had oral single primary carcinoma and 20 patients had oral multiple primary carcinomas. Oral multiple primary carcinomas showed female predilection and occurred more frequently in the lower gingiva and significantly less frequently in the tongue (P < 0.01). Oral multiple primary carcinomas showed a significantly higher recurrence rate (P < 0.01). The 5-year overall survival of oral single primary carcinoma patients was 88.0% compared with 95% for oral multiple primary carcinomas, with no significant difference (log rank test, P = 0.54). However, the 15-year survival rate dropped to 28.1% in oral multiple primary carcinomas. The cumulative disease incidence rates of metachronous second primary carcinoma from first carcinoma at 5 years and 10 years were 3.45% and 5.36%, respectively. [Conclusion] Oral multiple primary carcinomas rarely occur in the tongue. The 5-year survival rate showed no difference between single and multiple carcinoma patients, but over longer observation, the prognosis of multiple carcinoma was poor owing to a high recurrence rate. Because of the high recurrence rate and risk of further metachronous carcinoma in oral multiple primary carcinomas, longer-term follow-up is required

Two cases of Removal of Infected Hydroxyapatite after Filling in Remote Past

Hydroxyapatite （HA） has been used out as bone filling material in bone defects from various disease. Although there are some reports short-term postoperative infection of HA, there are few reports long-term postoperative infection of HA. We reported 2 cases of dental infection that HA filling region of mandible bone and removal of infected HA after long periods. One case who was underwent excision of cyst and apicoectomy and filled HA to bone defect one case resulting from excision of cyst of mandible twenty years ago. The other case who was underwent segmental resection of the mandible and reconstructed by reconstruction plate, HA block and pectoral major musculo-cutaneous flap because of cancer of floor of mouth twenty years ago. Both of two cases referred to our hospital because of swelling and pain in the same region and removed infected HA. There are still many cases filled HA to bone defect. In case we encounter the cases filled HA to bone defect, we need to pay attention to infection of HA and must call attention to the risk of HA to patients

Corrigendum to “Isothermal vapor-liquid equilibria of mixtures of (methanol + ethanol + 1-propanol or 2-propanol) at 333.15 K” (Fluid Phase Equil. (2000) 170 (1) (37–48) (S0378381200003137) (10.1016/S0378-3812(00)00313-7))

金沢大学理工研究域自然システム学系The authors regret typographical errors in Table 2 of the original paper. In particular, some values of phase mole fraction are incorrect. Table 2 should be read. [formula presented] The authors would like to apologise for any inconvenience caused. © 2017Erratu

An Empirical Method for Estimating Normal Boiling Point and other Physical Properties of Alkene Hydrocarbons

金沢大学工学部A method of estimating the structural variation in the boiling point and other physical properties of alkenes is developed. By this method, all properties are expressed in terms of a structural constant called the “effective carbon number” which depends on the number and relative position of double bonds and those of side chains but not on external variables such as the temperature. An empirical equation is presented to correlate the effective carbon number with molecular structure. By combining the use with the previously presented nomogram, it is proved to be quite useful for rapid evaluation of various properties including the temperature-vapor pressure relationship and the critical constants

Is the Importance of Achieving Stable Disease Different between Epidermal Growth Factor Receptor Tyrosine Kinase Inhibitors and Cytotoxic Agents in the Second-Line Setting for Advanced Non-small Cell Lung Cancer?

BackgroundIt is controversial whether achieving stable disease leads to a survival benefit and whether the importance of achieving stable disease differs between cytotoxic agents and molecular targeted agents. To examine these questions, the authors retrospectively reviewed phase II and III studies in the second-line setting for advanced non-small cell lung cancer using epidermal growth factor receptor (EGFR) tyrosine kinase inhibitors (TKIs) and cytotoxic agents separately.MethodsThe authors chose 45 trials for the chemotherapy group and nine for the EGFR TKI group by searching the PubMed database. All nine trials in the EGFR TKI group concern gefitinib and erlotinib.ResultsThe median survival time increased 0.0375 month with each 1% increase in stable disease rate (p = 0.039), and each 1% increase in response rate resulted in 0.0744 (p < 0.001) month of median survival time in the analysis combined with both cytotoxic agents and EGFR TKIs. Main and interaction terms for EGFR TKI treatment were not statistically significant. With respect to time to progression, only response rate showed a statistically significant relationship with survival.ConclusionsTo obtain response seems to be more important than to achieve stable disease for both cytotoxic agents and EGFR TKIs, although achieving stable disease is still valuable. The relationship between survival and response or stable disease appears similar for cytotoxic agents and EGFR TKIs

A 6-Year Controlled Gastric Adenocarcinoma Metastasized to the Lung, Cervical Spine and Mandible in a Japanese Male: A Patient Report

Gastric adenocarcinoma metastasized to the lung, cervical vertebrae and mandible 6 years after gastrectomy in a 70-year-old man. When the man visited our clinic, he complained of pain in the left mandible with paralysis in the left lower lip and diffuse swelling with a fluctuation inside the left ramus of the mandible. Medium contrast computed tomography (CT) presented bone loss that looked like a wormhole at the left angle of the mandible. Magnetic resonance imaging (MRI) revealed abscess or osteomyelitis at the site. He showed no response despite treatment with antibiotics, and we suspected a neoplastic lesion. With a mandibular ramus specimen obtained by biopsy and examined histopathologically, adenocarcinoma of the salivary gland was strongly suspected. MRI presented a neoplastic lesion in his cervical vertebrae, and by biopsy he was diagnosed with adenocarcinoma. Thereafter, chest CT presented multiple pulmonary metastases. Considering the patient’s history of gastrectomy due to gastric adenocarcinoma, the stomach, cervical vertebrae or mandible were examined pathologically and immunohistochemically by biopsy: all specimens showed a moderately differentiated type of tubular adenocarcinoma, and the results for cytokeratin-related tumor markers were the same. We finally diagnosed him as having metastases from gastric adenocarcinoma to the lung, cervical vertebrae and mandible. Because the metastases had spread to multiple organs, the mandibular lesion was not treated, and terminal care in another facility was unavoidably selected. In making a differential diagnosis of multiple metastases, pathological and immunohistochemical examinations of metastatic lesions by biopsy were very useful based on the diagnostic imagings by CT and MRI

The ASTRO-H X-ray Observatory

The joint JAXA/NASA ASTRO-H mission is the sixth in a series of highly successful X-ray missions initiated by the Institute of Space and Astronautical Science (ISAS). ASTRO-H will investigate the physics of the high-energy universe via a suite of four instruments, covering a very wide energy range, from 0.3 keV to 600 keV. These instruments include a high-resolution, high-throughput spectrometer sensitive over 0.3-2 keV with high spectral resolution of Delta E < 7 eV, enabled by a micro-calorimeter array located in the focal plane of thin-foil X-ray optics; hard X-ray imaging spectrometers covering 5-80 keV, located in the focal plane of multilayer-coated, focusing hard X-ray mirrors; a wide-field imaging spectrometer sensitive over 0.4-12 keV, with an X-ray CCD camera in the focal plane of a soft X-ray telescope; and a non-focusing Compton-camera type soft gamma-ray detector, sensitive in the 40-600 keV band. The simultaneous broad bandpass, coupled with high spectral resolution, will enable the pursuit of a wide variety of important science themes.Comment: 22 pages, 17 figures, Proceedings of the SPIE Astronomical Instrumentation "Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray

The Quiescent Intracluster Medium in the Core of the Perseus Cluster

Clusters of galaxies are the most massive gravitationally-bound objects in the Universe and are still forming. They are thus important probes of cosmological parameters and a host of astrophysical processes. Knowledge of the dynamics of the pervasive hot gas, which dominates in mass over stars in a cluster, is a crucial missing ingredient. It can enable new insights into mechanical energy injection by the central supermassive black hole and the use of hydrostatic equilibrium for the determination of cluster masses. X-rays from the core of the Perseus cluster are emitted by the 50 million K diffuse hot plasma filling its gravitational potential well. The Active Galactic Nucleus of the central galaxy NGC1275 is pumping jetted energy into the surrounding intracluster medium, creating buoyant bubbles filled with relativistic plasma. These likely induce motions in the intracluster medium and heat the inner gas preventing runaway radiative cooling; a process known as Active Galactic Nucleus Feedback. Here we report on Hitomi X-ray observations of the Perseus cluster core, which reveal a remarkably quiescent atmosphere where the gas has a line-of-sight velocity dispersion of 164+/-10 km/s in a region 30-60 kpc from the central nucleus. A gradient in the line-of-sight velocity of 150+/-70 km/s is found across the 60 kpc image of the cluster core. Turbulent pressure support in the gas is 4% or less of the thermodynamic pressure, with large scale shear at most doubling that estimate. We infer that total cluster masses determined from hydrostatic equilibrium in the central regions need little correction for turbulent pressure.Comment: 31 pages, 11 Figs, published in Nature July