A5043807571- Stellar, planetary, and galactic studies
- Astronomical Observations and Instrumentation
- Astronomy and Astrophysical Research
- Gamma-ray bursts and supernovae
- Astro and Planetary Science
- Fluid Dynamics Simulations and Interactions
- Historical Astronomy and Related Studies
- Inertial Sensor and Navigation
- Astrophysics and Star Formation Studies
- Fault Detection and Control Systems
- Archaeology and Historical Studies
- Fluid Dynamics and Heat Transfer
- Solar and Space Plasma Dynamics
- African history and culture analysis
- Ancient Egypt and Archaeology
- Space Exploration and Technology
- Molecular Spectroscopy and Structure
- Granular flow and fluidized beds
- Seismology and Earthquake Studies
- Astrophysical Phenomena and Observations
- 3D Modeling in Geospatial Applications
- Spacecraft and Cryogenic Technologies
- Architecture and Computational Design
- Calibration and Measurement Techniques
- Atmospheric Ozone and Climate
Bennetts Associates
2024
We performed a detailed spectroscopic analysis of three extremely metal-poor RR Lyrae stars, exploring uncharted territories at these low metallicities for this class stars. Using high-resolution spectra acquired with HARPS-N TNG, UVES VLT, and PEPSI LBT, employing Non-Local Thermodynamic Equilibrium (NLTE) spectral synthesis calculations, we provide abundance measurements Fe, Al, Mg, Ca, Ti, Mn, Sr. Our findings indicate that the stars have [Fe/H] = -3.40 \pm 0.05, -3.28 0.02, -2.77 0.05 HD...
Abstract The paper seeks to investigate novel potentials for building design and structure generation that arise at the intersection of computational AI-generated 3D geometries. Although use AI technologies is exponentially increasing inside architectural discipline, spatial configurations using geometries still limited in its applications represents an ongoing field investigation advanced research. In this regard, several questions need be answered: how can we new typologies from...
Theoretical Period-Age and Period-Age-Color relations for different chemical compositions have been recently derived using an updated homogeneous set of evolutionary pulsational models. We apply these to Cepheids in the Magellanic Clouds constrain recent star formation history dwarf galaxies. Finally, we also compare radial distribution classical with young clusters forming regions.
Direct measurements of Cepheid radii are a key for understanding the physical structure these variables, and in turn constraining their pulsation properties. In this paper we discuss numerical experiments performed testing accuracy obtained by adopting both pure Baade-Wesselink (BW) method revised CORS method, as well consistency assumptions on which methods based. We applied BW to synthetic light, color radial velocity curves predicted full amplitude, nonlinear, convective models at solar...