Simulations predict intermediate-mass black hole formation in globular clusters.

The formation process of intermediate-mass black holes (IMBHs), defined as those between 100 and 10 solar masses (), is debated. One potential origin is the growth of less-massive black holes merging with stars and compact objects within globular clusters (GCs). However, previous simulations have indicated that this process only produces IMBHs under 500 before gravitational wave recoil ejects them from the GC.

The origin of OB runaway stars.

About 20% of all massive stars in the Milky Way have unusually high velocities, the origin of which has puzzled astronomers for half a century. We argue that these velocities originate from strong gravitational interactions between single stars and binaries in the centers of star clusters. The ejecting binary forms naturally during the collapse of a young (≤1 million years old) star cluster.

Risk factors for oxaliplatin-induced hypersensitivity reactions in Japanese patients with advanced colorectal cancer.

Objective: Previously, we suggested that oxaliplatin (L-OHP)-related grade 3/4 hypersensitivity reactions occurred immediately after the initiation, but grade 1/2 reactions did not. This study was conducted to clarify the risk factors for L-OHP-related hypersensitivity reactions.

Methods: Clinical data from 108 Japanese patients with colorectal cancer were analyzed, who were treated with L-OHP-containing regimens, FOLFOX4 and/or mFOLFOX6.

[Micafungin therapy for a case of chronic necrotizing pulmonary aspergillosis].

The patient was a 42-year-old man who visited a physician with fever, and was diagnosed with pulmonary abscess. Antibiotic therapy was ineffective, and he was referred to our hospital. Chest CT scanning revealed a lesion with cavity formation with an infiltrative shadow in the right upper lobe, and another infiltrative shadow in the left upper lobe.

Solution structure of a tmRNA-binding protein, SmpB, from Thermus thermophilus.

Small protein B (SmpB) is required for trans-translation, binding specifically to tmRNA. We show here the solution structure of SmpB from an extremely thermophilic bacterium, Thermus thermophilus HB8, determined by heteronuclear nuclear magnetic resonance methods. The core of the protein consists of an antiparallel beta-barrel twisted up from eight beta-strands, each end of which is capped with the second or third helix, and the first helix is located beside the barrel.