Plasma membrane damage removal by F-actin-mediated shedding from repurposed filopodia

Repairing plasma membrane damage is vital to eukaryotic cell survival. Membrane shedding is thought to be key to this repair process, but a detailed view of how the process occurs is still missing. Here we used electron cryotomography to image the ultrastructural details of plasma membrane wound healing. We found that filopodia-like protrusions are built at damage sites, accompanied by retraction of neighboring filopodia, and that these repurposed protrusions act as scaffolds for membrane shedding. This suggests a new role for filopodia as reservoirs of membrane and actin for plasma membrane damage repair. Damage-induced shedding was dependent on F-actin dynamics and Myo1a, as well as Vps4B, an important component of the ESCRT machinery. Thus we find that damage shedding is more complex than current models of simple vesiculation from flat membrane domains. Rather, we observe structural similarities between damage-mediated shedding and constitutive shedding from enterocytes that argue for conservation of a general membrane shedding mechanism

Stable sub-complexes observed in situ suggest a modular assembly pathway of the bacterial flagellar motor

The self-assembly of cellular macromolecular machines such as the bacterial flagellar motor requires the spatio- temporal synchronization of gene expression, protein localization and association of a dozen or more unique components. In Salmonella and Escherichia coli, a sequential, outward assembly mechanism has been proposed for the flagellar motor starting from the inner membrane, with each subsequent component stabilizing the last. Here, using electron cryo-tomography of intact Legionella pneumophila, Pseudomonas aeruginosa and Shewanella oneidensis cells, we observe stable outer-membrane-embedded sub-complexes of the flagellar motor. These sub- complexes consist of the periplasmic embellished P- and L-rings, in the absence of other flagellar components, and bend the membrane inward dramatically. Additionally, we also observe independent inner-membrane sub- complexes consisting of the C- and MS-rings and export apparatus. These results suggest an alternate model for flagellar motor assembly in which outer- and inner-membrane-associated sub-complexes form independently and subsequently join, enabling later steps of flagellar production to proceed

Upper Limits on a Stochastic Background of Gravitational Waves

The Laser Interferometer Gravitational-Wave Observatory has performed a third science run with much improved sensitivities of all three interferometers. We present an analysis of approximately 200 hours of data acquired during this run, used to search for a stochastic background of gravitational radiation. We place upper bounds on the energy density stored as gravitational radiation for three different spectral power laws. For the flat spectrum, our limit of Ω_0<8.4×10^(-4) in the 69–156 Hz band is ~10^5 times lower than the previous result in this frequency range

Limits on Gravitational-Wave Emission from Selected Pulsars Using LIGO Data

We place direct upper limits on the amplitude of gravitational waves from 28 isolated radio pulsars by a coherent multidetector analysis of the data collected during the second science run of the LIGO interferometric detectors. These are the first direct upper limits for 26 of the 28 pulsars. We use coordinated radio observations for the first time to build radio-guided phase templates for the expected gravitational-wave signals. The unprecedented sensitivity of the detectors allows us to set strain upper limits as low as a few times 10^(-24). These strain limits translate into limits on the equatorial ellipticities of the pulsars, which are smaller than 10^(-5) for the four closest pulsars

First search for gravitational waves from the youngest known neutron star

We present a search for periodic gravitational waves from the neutron star in the supernova remnant Cassiopeia A. The search coherently analyzes data in a 12 day interval taken from the fifth science run of the Laser Interferometer Gravitational-Wave Observatory. It searches gravitational-wave frequencies from 100 to 300 Hz and covers a wide range of first and second frequency derivatives appropriate for the age of the remnant and for different spin-down mechanisms. No gravitational-wave signal was detected. Within the range of search frequencies, we set 95% confidence upper limits of (0.7–1.2) × 10^(−24) on the intrinsic gravitational-wave strain, (0.4–4) × 10^(−4) on the equatorial ellipticity of the neutron star, and 0.005–0.14 on the amplitude of r-mode oscillations of the neutron star. These direct upper limits beat indirect limits derived from energy conservation and enter the range of theoretical predictions involving crystalline exotic matter or runaway r-modes. This paper is also the first gravitational-wave search to present upper limits on the r-mode amplitude