Results 171 to 180 of about 50,322 (326)
Kinematics and simulations of the stellar stream in the halo of the Umbrella Galaxy [PDF]
Caroline Foster +11 more
openalex +1 more source
Origami‐Inspired Structural Design for Aquatic‐Terrestrial Amphibious Robots
This work presents a lightweight amphibious origami robot actuated by a single shape memory alloy wire. A rigid foldable origami structure with displacement amplification enables efficient terrestrial crawling and aquatic swimming. The addition of fan‐shaped units allows controllable turning in both environments.
Weiqi Liu +5 more
wiley +1 more source
Star formation in early-type galaxies: the role of stellar winds and kinematics [PDF]
Silvia Pellegrini +2 more
openalex +1 more source
Phase‐field method based numerical modelling of the capillary rise in millimeter‐sized tubes, aiming for anti‐slip applications. The experimental validation was performed through capillary assays in polyethylene oxide (PEO) bulk modified polydimethylsiloxane (PDMS) channels.
Shivam Sharma +7 more
wiley +1 more source
LOCAL GROUP DWARF ELLIPTICAL GALAXIES. II. STELLAR KINEMATICS TO LARGE RADII IN NGC 147 AND NGC 185 [PDF]
Marla Geha +5 more
openalex +1 more source
Stellar kinematics in disk galaxies
n this thesis several aspects of the stellar kinematics in disk galaxies have been addressed. Due to the low surface brightness of these systems the number of studies that have addressed these issues has been fairly limited. However, kinematic studies, especially stellar kinematics because stars make up the bulk of a galaxy's visible matter, remain ...
openaire +1 more source
EGF‐induced de novo transcription of connexins Cx26 and Cx31 promotes flocking behavior that fluidizes epithelia and enables coordinated collective migration. Connexin‐driven cytoplasmic exchange mechanistically links growth‐factor signaling to invasive dynamics.
Hind Abdo +18 more
wiley +1 more source
The Milky Way (MW) is a barred spiral galaxy shaped by tidal interactions with its satellites. The Large Magellanic Cloud (LMC) and the Sagittarius dwarf galaxy (Sgr) are the dominant influences at the present day. This paper presents a suite of four 10 ^
Ioana A. Stelea +2 more
doaj +1 more source
The benchmark black hole in NGC 4258: dynamical models from high-resolution two-dimensional stellar kinematics [PDF]
Daniel Alf Drehmer +4 more
openalex +1 more source
The stellar halos of ETGs in the IllustrisTNG simulations: The photometric and kinematic diversity of galaxies at large radii [PDF]
C. Pulsoni +6 more
openalex +1 more source

