Results 121 to 130 of about 27,475,594 (335)
In situ molecular organization and heterogeneity of the Legionella Dot/Icm T4SS
We present a nearly complete in situ model of the Legionella Dot/Icm type IV secretion system, revealing its central secretion channel and identifying new components. Using cryo‐electron tomography with AI‐based modeling, our work highlights the structure, variability, and mechanism of this complex nanomachine, advancing understanding of bacterial ...
Przemysław Dutka +11 more
wiley +1 more source
GravSphere2: A higher order Jeans method for mass modeling spherical stellar systems
Aims. Mass-modeling methods are used to infer the gravitational field of stellar systems, from globular clusters to giant elliptical galaxies. While many methods already exist, most require assumptions on the form of the underlying distribution function ...
Bañares-Hernández Andrés +2 more
doaj +1 more source
The author calls a topological group \(G\) \(\tau\)\textit{-locally invariant,} where \(\tau\) is an infinite cardinal, if \(G\) embeds, as a topological subgroup, into the direct product of a family of topological groups of character \(
openaire +1 more source
We introduce the category of locally C-Nash groups, basic examples of such groups are complex algebraic groups. We prove that the latter form a full subcategory. We also show that both, abelian locally Nash and abelian locally C-Nash groups, can be characterised via meromorphic maps admitting an algebraic addition theorem; we give an invariant of such ...
Baro, Elías +2 more
openaire +3 more sources
We reconstituted Synechocystis glycogen synthesis in vitro from purified enzymes and showed that two GlgA isoenzymes produce glycogen with different architectures: GlgA1 yields denser, highly branched glycogen, whereas GlgA2 synthesizes longer, less‐branched chains.
Kenric Lee +3 more
wiley +1 more source
WLM: Dynamics of an isolated dwarf irregular galaxy under ram pressure in the Local Group
The Wolf–Lundmark–Melotte (WLM) galaxy is an archetypal dwarf irregular galaxy that has not experienced interactions with major Local Group galaxies within the past 8 Gyr.
Kolhe Neel +7 more
doaj +1 more source
Let \(G\) be a group, \(H \leq G\), \(\mathcal C\) the conjugacy class of \(H\) in \(G\), \(k\) a field of characteristic \(p\), \(V\) a \(kG\)-module. Let \(^H V=\{v \in V :\) for all \(h \in H\), \(hv=v\}\), \(S(V)=\sum_{K \neq 1} {^KV}\), \(Q(V)=V/S(V)\), \(S^H(V)=\sum_{K\in{\mathcal C}} {^KV}\), \(Q^{(H)}(V)=V/S^{(H)}(V)\). \(G\) is \(p\)-smooth \(\
openaire +3 more sources
Structural biology of ferritin nanocages
Ferritin is a conserved iron‐storage protein that sequesters iron as a ferric mineral core within a nanocage, protecting cells from oxidative damage and maintaining iron homeostasis. This review discusses ferritin biology, structure, and function, and highlights recent cryo‐EM studies revealing mechanisms of ferritinophagy, cellular iron uptake, and ...
Eloise Mastrangelo, Flavio Di Pisa
wiley +1 more source
Estimating the dynamical masses of dwarf galaxies in the presence of binary-star contamination
Context. The line-of-sight (l.o.s.) velocity dispersion (σlos) of the stellar component of ultra-faint-dwarf galaxies (UFDs) typically ranges from 3 to 6 km s−1. Applying standard mass estimators, this hints at extreme dynamical mass-to-light ratios (M/L)
Arroyo-Polonio José María +2 more
doaj +1 more source

