Results 111 to 120 of about 6,735 (287)
The history, current state and future directions of the three MX beamlines BL14.1, BL14.2 and BL14.3 of the Helmholtz‐Zentrum Berlin at the BESSY II electron storage ring are described.Since 2003, the Macromolecular Crystallography (MX) group at Helmholtz‐Zentrum Berlin (HZB) has been operating three MX beamlines at the BESSY II storage ring in Berlin.
Uwe Mueller+18 more
wiley +1 more source
Liquid metallic hydrogen and the structure of brown dwarfs and giant planets [PDF]
W. B. Hubbard+6 more
openalex +1 more source
Revealing giant planet interiors beneath the cloudy veil. [PDF]
Guillot T, Fletcher LN.
europepmc +1 more source
A Smithian Political Economy Approach for the Competition Law of the 21st Century
This study aims to show how a Smithian political economy approach could assist competition law in addressing the challenges of the 21st‐century economy. We revisit Smith's Wealth of Nations to provide a more nuanced understanding of his views, contrasting them with the prevailing libertarian interpretation called here ‘Chicago Smith’.
Stavros Makris
wiley +1 more source
Prospects for detection of extra-solar giant planets by next-generation telescopes [PDF]
Adam Burrows+4 more
openalex +1 more source
How Well Do We Understand the Belt/Zone Circulation of Giant Planet Atmospheres? [PDF]
Fletcher LN+3 more
europepmc +1 more source
Our findings reveal that the western black crested gibbon (Nomascus concolor) did not divide into different subspecies, and the relatively low level of genetic diversity emphasizes the importance of monitoring this indicator for vulnerable wildlife.
Siqiong LIU+15 more
wiley +1 more source
Accelerating Giant-impact Simulations with Machine Learning
Constraining planet-formation models based on the observed exoplanet population requires generating large samples of synthetic planetary systems, which can be computationally prohibitive.
Caleb Lammers+5 more
doaj +1 more source
We confirm TOI-4201 b as a transiting Jovian-mass planet orbiting an early M dwarf discovered by the Transiting Exoplanet Survey Satellite. Using ground-based photometry and precise radial velocities from NEID and the Planet Finder Spectrograph, we ...
Megan Delamer+29 more
doaj +1 more source
Formation of Giant Planets: Dependences on Core Accretion Rate and Grain Opacity [PDF]
Masahiro Ikoma+2 more
openalex +1 more source