flare star वाक्य
उदाहरण वाक्य
मोबाइल
- It has a greater luminosity than most flare stars, which are typically red dwarfs, but is less active.
- Both members are flare stars, meaning they are red dwarf stars that undergo random eruptions that increase their brightness.
- This group includes protostars, Wolf-Rayet stars, and flare stars, as well as giant and supergiant stars.
- However, like the star UV Ceti, it has been observed to undergo increases in luminosity as a flare star.
- In 1958 it was thought to have stellar companion that was also a flare star, but this was subsequently disproved.
- At other times, some red dwarfs, called flare stars, can emit gigantic flares, doubling their brightness in minutes.
- He provided the data that lead to Willem Jacob Luyten's discovery of UV Ceti, the first known flare star.
- This was a discovery made in his earliest work on flare stars and solar-related phenomena which he pioneered at Armagh Observatory.
- NPOI is one of the few major instruments globally which can conduct stellar disks ( the first in history ) and flare stars.
- It is classified as an active flare star since it can undergo unpredictable and dramatic increases in luminosity for a period of several minutes.
- Red dwarfs and brown dwarfs exhibit two main forms of variability : they could be BY Draconis variables or flare stars, or both.
- Flare stars can increase in brightness by a few magnitudes in just a few minutes, and fade to normal in a few hours.
- It is a flare star, emitting unpredictable outbursts of energy for mere minutes, which might be much more powerful analogues of solar flares.
- Wolf 359 is a red dwarf of magnitude 13.5; it periodically brightens by one magnitude or less because it is a flare star.
- It is common only among the flare stars, also known as the UV Ceti variables, very faint main-sequence stars which undergo regular flares.
- In 1969, a brief flare in the luminosity of Wolf 359 was observed, linking it to the class of variable stars known as flare stars.
- From 1984 he was actively engaged in the search for quasi-periodic ultraviolet and infrared variations in flare stars indicative of active regions and stellar rotation.
- AD Leonis is a main sequence star with a spectral classification of M3.5V . It is a flare star that undergoes random increases in luminosity.
- It is a flare star that can emit powerful flares potentially visible to the naked eye, thousands of times more energetic than any from Earth's sun.
- His master's degree is from the University of Toledo, based on studies he did at Kitt Peak Observatory of eruptive and flare stars among red dwarfs.
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