Phosphoinositide-binding interface proteins involved in shaping cell membranes

The mechanism by which cell and cell membrane shapes are created has long been a subject of great interest. Among the phosphoinositide-binding proteins, a group of proteins that can change the shape of membranes, in addition to the phosphoinositide-binding ability, has been found. These proteins, which contain membrane-deforming domains such as the BAR, EFC/F-BAR, and the IMD/I-BAR domains, led to inward-invaginated tubes or outward protrusions of the membrane, resulting in a variety of membrane shapes. Furthermore, these proteins not only bind to phosphoinositide, but also to the N-WASP/WAVE complex and the actin polymerization machinery, which generates a driving force to shape the membranes

Gamendazole, an Orally Active Indazole Carboxylic Acid Male Contraceptive Agent, Targets HSP90AB1 (HSP90BETA) and EEF1A1 (eEF1A), and Stimulates Il1a Transcription in Rat Sertoli Cells

Gamendazole was recently identified as an orally active antispermatogenic compound with antifertility effects. The cellular mechanism(s) through which these effects occur and the molecular target(s) of gamendazole action are currently unknown. Gamendazole was recently designed as a potent orally active antispermatogenic male contraceptive agent. Here, we report the identification of binding targets and propose a testable mechanism of action for this antispermatogenic agent. Both HSP90AB1 (previously known as HSP90beta [heat shock 90-kDa protein 1, beta]) and EEF1A1 (previously known as eEF1A [eukaryotic translation elongation factor 1 alpha 1]) were identified as binding targets by biotinylated gamendazole (BT-GMZ) affinity purification from testis, Sertoli cells, and ID8 ovarian cancer cells; identification was confirmed by matrix-assisted laser desorption/ionization-time of flight mass spectrometry and Western blot analysis. BT-GMZ bound to purified yeast HSP82 (homologue to mammalian HSP90AB1) and EEF1A1, but not to TEF3 or HBS1, and was competed by unlabeled gamendazole. However, gamendazole did not inhibit nucleotide binding by EEF1A1. Gamendazole binding to purified Saccharomyces cerevisiae HSP82 inhibited luciferase refolding and was not competed by the HSP90 drugs geldanamycin or novobiocin analogue, KU-1. Gamendazole elicited degradation of the HSP90-dependent client proteins AKT1 and ERBB2 and had an antiproliferative effect in MCF-7 cells without inducing HSP90. These data suggest that gamendazole may represent a new class of selective HSP90AB1 and EEF1A1 inhibitors. Testis gene microarray analysis from gamendazole-treated rats showed a marked, rapid increase in three interleukin 1 genes and Nfkbia (NF-kappaB inhibitor alpha) 4 h after oral administration. A spike in II1a transcription was confirmed by RT-PCR in primary Sertoli cells 60 min after exposure to 100 nM gamendazole, demonstrating that Sertoli cells are a target. AKT1, NFKB, and interleukin 1 are known regulators of the Sertoli cell-spermatid junctional complexes. A current model for gamendazole action posits that this pathway links interaction with HSP90AB1 and EEF1A1 to the loss of spermatids and resulting infertility

Observation of Gravitational Waves from the Coalescence of a 2.5−4.5 M⊙2.5-4.5~M_\odot Compact Object and a Neutron Star

International audienceWe report the observation of a coalescing compact binary with component masses $2.5-4.5~M_\odot$ and $1.2-2.0~M_\odot$ (all measurements quoted at the 90% credible level). The gravitational-wave signal GW230529_181500 was observed during the fourth observing run of the LIGO-Virgo-KAGRA detector network on 2023 May 29 by the LIGO Livingston Observatory. The primary component of the source has a mass less than $5~M_\odot$ at 99% credibility. We cannot definitively determine from gravitational-wave data alone whether either component of the source is a neutron star or a black hole. However, given existing estimates of the maximum neutron star mass, we find the most probable interpretation of the source to be the coalescence of a neutron star with a black hole that has a mass between the most massive neutron stars and the least massive black holes observed in the Galaxy. We estimate a merger rate density of $55^{+127}_{-47}~\text{Gpc}^{-3}\,\text{yr}^{-1}$ for compact binary coalescences with properties similar to the source of GW230529_181500; assuming that the source is a neutron star-black hole merger, GW230529_181500-like sources constitute about 60% of the total merger rate inferred for neutron star-black hole coalescences. The discovery of this system implies an increase in the expected rate of neutron star-black hole mergers with electromagnetic counterparts and provides further evidence for compact objects existing within the purported lower mass gap