Results 101 to 110 of about 1,100,727 (344)
Peptide‐based ligand antagonists block a Vibrio cholerae adhesin
The structure of a peptide‐binding domain of the Vibrio cholerae adhesin FrhA was solved by X‐ray crystallography, revealing how the inhibitory peptide AGYTD binds tightly at its Ca2+‐coordinated pocket. Structure‐guided design incorporating D‐amino acids enhanced binding affinity, providing a foundation for developing anti‐adhesion therapeutics ...
Mingyu Wang +9 more
wiley +1 more source
Constraining Stellar Winds of Young Sun-like Stars
As part of the project Pathways to Habitability (http://path.univie.ac.at/), we study the properties of the stellar winds of low-mass and Sun-like stars, and their influences on the atmospheres of potentially habitable planets.
Fichtinger, Bibiana +3 more
core +1 more source
The Solar--Stellar Connection [PDF]
Stars have proven to be surprisingly prolific radio sources and the added sensitivity of the Square Kilometer Array will lead to advances in many directions.
Anglada +42 more
core +2 more sources
Clumped stellar winds in supergiant high‐mass X‐ray binaries: X‐ray variability and photoionization [PDF]
The clumping of massive star winds is an established paradigm confirmed by multiple lines ofevidence and supported by stellar wind theory. The purpose of this paper is to bridge the gapbetween detailed models of inhomogeneous stellar winds in single stars
L. Oskinova, A. Feldmeier, P. Kretschmar
semanticscholar +1 more source
There is an unmet need in metastatic breast cancer patients to monitor therapy response in real time. In this study, we show how a noninvasive and affordable strategy based on sequencing of plasma samples with longitudinal tracking of tumour fraction paired with a statistical model provides valuable information on treatment response in advance of the ...
Emma J. Beddowes +20 more
wiley +1 more source
A Blind Search for Magnetospheric Emissions from Planetary Companions to Nearby Solar-type Stars
This paper reports a blind search for magnetospheric emissions from planets around nearby stars. Young stars are likely to have much stronger stellar winds than the Sun, and because planetary magnetospheric emissions are powered by stellar winds ...
Aubier +33 more
core +1 more source
Really focused stellar winds in X-ray binaries [PDF]
Aims. We investigate the anisotropy of stellar winds in binaries to improve the models of accretion in high-mass X-ray binaries. Methods. We model numerically the stellar wind from a supergiant component of a binary in radial and three-dimensional ...
P. Hadrava, Jan vCechura
semanticscholar +1 more source
This study used longitudinal transcriptomics and gene‐pattern classification to uncover patient‐specific mechanisms of chemotherapy resistance in breast cancer. Findings reveal preexisting drug‐tolerant states in primary tumors and diverse gene rewiring patterns across patients, converging on a few dysregulated functional modules. Despite receiving the
Maya Dadiani +14 more
wiley +1 more source
Comprehensive analysis of genomic mutations, gene expression, DNA methylation, and pathway analysis of TCGA data was carried out to define cancer types in which proteasome subunits expression is associated with worse survival. Albeit the effect of specific proteasome subunits on cellular function, the main role of the proteasome is better evaluated ...
Ruba Al‐Abdulla +5 more
wiley +1 more source
Testing the Rossby Paradigm: Weakened Magnetic Braking in Early K-type Stars
There is an intricate relationship between the organization of large-scale magnetic fields by a stellar dynamo and the rate of angular momentum loss due to magnetized stellar winds. An essential ingredient for the operation of a large-scale dynamo is the
Travis S. Metcalfe +14 more
doaj +1 more source

