Results 101 to 110 of about 1,401,162 (283)
Plastic and Reconstructive Surgery, Global Open, 2020 Edward M. Gronet, MD +3 more
doaj +1 more source
Open Astronomy, 2010 The spectroscopic orbit of a high proper motion star, BD+20 5152, is calculated from 34 CORAVEL-type radial velocity measurements. The star has a slightly eccentric orbit with a period of 5.70613 d, half-amplitude of 47.7 km/s and eccentricity of 0.049 ...
Sperauskas J. +3 more
doaj +1 more source
Retired A Stars and Their Companions. IV. Seven Jovian Exoplanets from Keck Observatory1 [PDF]
, 2010 John Asher Johnson +7 more
openalex +1 more source
FEBS Letters, EarlyView.Cells must clear mislocalized or faulty proteins from membranes to survive. The AAA+ ATPase Msp1 performs this task, but dissecting how its six subunits work together is challenging. We engineered linked dimers with varied numbers of functional subunits to reveal how Msp1 subunits cooperate and use energy to extract proteins from the lipid bilayer ...
Deepika Gaur +5 more
wiley +1 more source
Open Astronomy, 2011 The chemi-ionization processes in atom - Rydberg atom collisions, as well as the corresponding chemi-recombination processes, are considered as factors of influence on the atom exited-state populations in weakly ionized layers of stellar atmospheres. The
Mihajlov Anatolij A. +3 more
doaj +1 more source
Organoids in pediatric cancer research
FEBS Letters, EarlyView.Organoid technology has revolutionized cancer research, yet its application in pediatric oncology remains limited. Recent advances have enabled the development of pediatric tumor organoids, offering new insights into disease biology, treatment response, and interactions with the tumor microenvironment.
Carla Ríos Arceo, Jarno Drost
wiley +1 more source
Modeling of the Continuous Absorption of Electromagnetic Radiation in Dense Hydrogen Plasma
Open Astronomy, 2011 We investigate a new modeling way for describing the continuous absorption of electromagnetic radiation in a dense partially ionized hydrogen plasma with electron densities 5·1018-1.5·1019 cm-3 and temperatures 16 000–25 000 K, in the wavelength range ...
Mihajlov A. A. +3 more
doaj +1 more source
, 2016 The origin of carbon-enhanced metal-poor (CEMP) stars plays a key role in characterising the formation and evolution of the first stars and the Galaxy since the extremely-poor (EMP) stars with [Fe/H] \leq -2.5 share the common features of carbon ...
Fujimoto, Masayuki Y. +2 more
core +1 more source
The mass–radius relationship for very low mass stars: four new discoveries from the HATSouth Survey★ [PDF]
, 2013 George Zhou +17 more
openalex +1 more source