The authors re-examine the galactic kinematics of relic galaxy NGC 1277, recently identified as dark matter deficient, by reproducing its rotation curve with data from the George and Cynthia Mitchell Spectrograph.
Read More...Examination of the rotation curve for the dark matter deficient relic galaxy NGC 1277
The authors re-examine the galactic kinematics of relic galaxy NGC 1277, recently identified as dark matter deficient, by reproducing its rotation curve with data from the George and Cynthia Mitchell Spectrograph.
Read More...Visualizing black holes and wormholes through raytracing
The authors visualized black holes and wormholes using code and ray-tracing programs.
Read More...Exploration of the density–size correlation of celestial objects on various scales
Building on previous work by earlier astronomers, the authors investigate the correlation between the density and size of celestial objects in the universe, including neutron stars, galaxies, and galaxy clusters.
Read More...Disputing the green valley theory of galaxy evolution
Exploring the resonant vibration of a cello with the finite element method
The effect of circumference on the segregation of objects in a mixture
The authors test how the size-segregation theory applies to the behavior of hollow and irregular-shaped objects.
Read More...Calculating the dynamic viscosity of a fluid using image processing of a falling ball
The authors measure changes in the viscosity of glycerol with increasing temperature using the falling ball approach.
Read More...Generation of a magnetic field on Mars
The authors propose and test a method that would allow for the generation of a magnetic field on Mars sufficient to support future colonization.
Read More...Investigating momentum transfer with gall-forming wasps
The authors use the unique movements of the jumping gall wasp to study momentum transfer with potential applications in robotics and extraterrestrial research.
Read More...Photometric analysis of Type Ia Supernova 2023jvj
Here the authors conducted a photometric analysis of Supernova (SN) 20234jvj. Through generating a light curve, they determined SN 2023jvj to be a Type Ia supernova located approximately 1.246e8 parasecs away from Earth.
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