10,886 research outputs found

    Signal regulatory protein alpha expression and function in human vascular endothelium

    Full text link
    Thesis (M.A.)--Boston UniversityThe human immune system is capable of detecting and removing foreign invaders such as viruses, microorganisms, and other harmful materials. A key component of this immune response is leukocyte recruitment—a process, in which leukocytes travel from the bloodstream to the site of injury or infection. SIRPα, a protein mainly known to be expressed in myeloid leukocytes, has been shown to contribute to this process by regulating transendothelial migration (TEM)—leukocyte passage through the vascular endothelium. Interestingly, a recent study has detected low levels of SIRPα on surface of cultured endothelial cells. The aim of this study was to confirm endothelial expression of SIRPα and to investigate its role in leukocyte TEM. SIRPα expression on the endothelial cell was confirmed by immunofluorescence microscopy, indirect immunofluorescence and flow cytometry, and by western blot analysis. shRNA silencing and function blocking antibodies were used to block the adhesive function of SIRPα in an in vitro TEM assay under physiological shear flow conditions. The interventions did not alter leukocyte TEM and we conclude that SIRPα does not play a significant role in leukocyte TEM in vitro

    OPA1 processing controls mitochondrial fusion and is regulated by mRNA splicing, membrane potential, and Yme1L

    Get PDF
    OPA1, a dynamin-related guanosine triphosphatase mutated in dominant optic atrophy, is required for the fusion of mitochondria. Proteolytic cleavage by the mitochondrial processing peptidase generates long isoforms from eight messenger RNA (mRNA) splice forms, whereas further cleavages at protease sites S1 and S2 generate short forms. Using OPA1-null cells, we developed a cellular system to study how individual OPA1 splice forms function in mitochondrial fusion. Only mRNA splice forms that generate a long isoform in addition to one or more short isoforms support substantial mitochondrial fusion activity. On their own, long and short OPA1 isoforms have little activity, but, when coexpressed, they functionally complement each other. Loss of mitochondrial membrane potential destabilizes the long isoforms and enhances the cleavage of OPA1 at S1 but not S2. Cleavage at S2 is regulated by the i-AAA protease Yme1L. Our results suggest that mammalian cells have multiple pathways to control mitochondrial fusion through regulation of the spectrum of OPA1 isoforms

    Black Hole Hyperaccretion Inflow-outflow Model. I. Long And Ultra-long Gamma-ray Bursts

    Full text link
    Long-duration gamma-ray bursts (LGRBs) and ultra-LGRBs (ULGRBs) originate from collapsars, in the center of which a newborn rotating stellar-mass black hole (BH) surrounded by a massive accretion disk may form. In the scenario of the BH hyperaccretion inflow-outflow model and Blandford-Znajek (BZ) mechanism to trigger gamma-ray bursts (GRBs), the real accretion rate to power a BZ jet is far lower than the mass supply rate from the progenitor star. The characteristics of the progenitor stars can be constrained by GRB luminosity observations, and the results exceed usual expectations. LGRBs lasting from several seconds to tens of seconds in the rest frame may originate from solar-metallicity (Z ∼ 1 Z⊙, where Z and Z⊙ are the metallicities of progenitor stars and the Sun), massive (M ≳ 34 M⊙, where M and M⊙ are the masses of progenitor stars and the Sun) stars or some zerometallicity (Z ∼ 0) stars. A fraction of low-metallicity (Z ≲ 10-2Z⊙) stars, including Population III stars, can produce ULGRBs such as GRB 111209A. The fraction of LGRBs lasting less than tens of seconds in the rest frame is more than 40%, which cannot conform to the fraction of the demanded type of progenitor star. It possibly implies that the activity timescale of the central engine may be much longer than the observed timescale of prompt emission phase, as indicated by X-ray late-time activities. Alternatively, LGRBs and ULGRBs may be powered by a millisecond magnetar central engine. © 2017. The American Astronomical Society. All rights reserved
    • …
    corecore