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Full-Text Articles in Physical Sciences and Mathematics
The Critical Parameters Of A Slowly Rotating Neutron Star, Vildyan Yanbikov
The Critical Parameters Of A Slowly Rotating Neutron Star, Vildyan Yanbikov
Vildyan Yanbikov
A model of unstable conditions of a slowly rotating neutron star. The formulas for calculating the mass and diameter of a neutron star. As well as the pressure and temperature in the center of the star. At the time of its unstable condition before it exploded.
Unmasking The Mysteries Of High-Mass X-Ray Binaries (Hmxbs): The Role Of The Electron Beam Ion Trap (Ebit), Carey L. Baxter, Greg Brown, Natalie Hell
Unmasking The Mysteries Of High-Mass X-Ray Binaries (Hmxbs): The Role Of The Electron Beam Ion Trap (Ebit), Carey L. Baxter, Greg Brown, Natalie Hell
Carey L Baxter
The Electron Beam Ion Trap (EBIT) uses a very narrow electron beam (~60μm) to excite and trap ions. X-ray emissions of the excited ions are then diffracted and analyzed. I studied specific spectral emission lines of ionized silicon. This data can be used as a point of reference for similar spectra measured by the satellite Chandra so that the Doppler shift due to wind around the accretion disks of High Mass X-ray Binaries (HMXBs) can be calculated. HMXBs are pairs of stars that are luminous in X-rays. They are composed of a donor star that gives up mass to an …