- Quasar Framework
Developer-oriented, front-end framework with VueJS components for best-in-class high-performance, responsive websites, PWA, SSR, Mobile and Desktop apps, all from the same codebase Sensible people choose Vue Productive people choose Quasar Be both
- GitHub - quasar Quasar: Remote Administration Tool for Windows
Free, Open-Source Remote Administration Tool for Windows Quasar is a fast and light-weight remote administration tool coded in C# The usage ranges from user support through day-to-day administrative work to employee monitoring
- Quasar | Discovery, Structure Evolution | Britannica
Quasar, an astronomical object of very high luminosity found in the centres of some galaxies and powered by gas spiraling at high velocity into an extremely large black hole
- Quasars — Everything you need to know about the brightest objects in . . .
Quasars are the remarkably bright cores of active galaxies in the distant universe, they are an extreme form of what astronomers call "active galactic nuclei", or AGN for short
- Quasar – Definition, Formation, Facts in Astronomy
A quasar, short for “quasi-stellar radio source,” is the brightest and most energetic object in the universe Quasars are the active cores of distant galaxies, powered by supermassive black holes devouring surrounding matter
- What is a quasar? - EarthSky
The word quasar stands for quasi-stellar radio source Quasars got that name because they looked starlike when astronomers first began to notice them in the late 1950s and early 60s
- Hubble Quasars - NASA Science
Among its quasar observations, in 2019 Hubble found the brightest quasar known in the early universe by using a combination of its sharp vision and a natural gravitational lens in space to see the distant object
- Quasar - ESA Hubble
Quasars are amongst the most luminous objects in the known Universe, typically emitting thousands of times more light than the entire Milky Way They are distinguished from other AGNs by their enormous luminosity, and their enormous distances from Earth
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