Results 41 to 50 of about 412,900 (233)
Multi-dimensional simulations of bow shocks of massive, high-velocity runaway stars [PDF]
Stellar bow shocks result from the supersonic collision of stellar winds ejected by runaway stars and the interstellar medium (ISM). Studying their properties provides constraints on mass-loss rates, stellar wind velocities and the properties of the ISM.
Ramalatswa, Katlego Jafta
core +1 more source
Spindown of Pulsars Interacting with Companion Winds: The Impact of Magnetospheric Compression
Pulsars in binary systems with strong companion winds can have the magnetopause separating their magnetosphere from the wind located well within their light cylinder.
Yici Zhong +3 more
doaj +1 more source
OsCPK12‐OsATPD1 Module Regulates Photosynthetic Acclimation to Light Stress in Rice
OsCPK12 interacts and phosphorylates OsAtpD1 at Ser8 in its transit peptide. This phosphorylation promote its chloroplast translocation, thereby maintaining ATP synthase activity and proton gradient (ΔpH) homeostasis and regulating photosynthetic acclimation, photoprotection, and repair under light stress.
Beifang Wang +17 more
wiley +1 more source
The JWST-NIRCam View of Sagittarius C. I. Massive Star Formation and Protostellar Outflows
We present James Webb Space Telescope (JWST) Near Infrared Camera observations of the massive star-forming molecular cloud Sagittarius C (Sgr C) in the Central Molecular Zone (CMZ).
Samuel Crowe +16 more
doaj +1 more source
AM symbiosis induces GhWAK13 to promote fungal colonization. GhNTF3 negatively regulates symbiosis by promoting SA biosynthesis. GhWAK13 sequesters GhNTF3 at the membrane, limiting its nuclear translocation and relieving SA‐mediated suppression. Under Verticillium stress, GhNTF3 enters the nucleus and interacts with GhJAZ6 to activate SA signaling ...
Shuangjie Jia +10 more
wiley +1 more source
Streams and Bubbles: Tidal Shaping of Hydrodynamic Planetary Outflows
Planets, especially those close to their host stars, lose mass to atmospheric outflows, a process that is thought to shape the bimodal population of gaseous giant and rocky terrestrial exoplanets in close orbits.
Morgan MacLeod +3 more
doaj +1 more source
Large-scale emission from γ-ray binaries: the case of LS 5039
Context. Gamma-ray binaries hosting a non-accreting neutron star and a massive star exhibit multi-wavelength emission on different spatial scales.
Martinez J. R., Bosch-Ramon V.
doaj +1 more source
A Synthetic Platform for Antibody Junctional Diversification Beyond Natural Constraints
ARESEC is a synthetic platform that reconstructs functional V(D)J recombination in HEK293T cells. By introducing RSS elements and co‐expressing RAG1/2 and TdT across all three antibody CDRs, it enables programmable junctional diversification and direct generation of high‐affinity variants targeting PD‐1/PD‐L1, overcoming the evolutionary constraints of
Wang Liu +3 more
wiley +1 more source
Interstellar Ultraviolet Lyα High Resolution Mapping from the New Horizons P-Alice Instrument
We present New Horizons Alice spectral observations of interstellar hydrogen Ly α emissions at a vantage point of 57 au from the Sun. The observations were conducted as a pair of orthogonal scans to produce high spatial angular resolution measurements of
Tracy M. Becker +19 more
doaj +1 more source

