T Tauri is a variable star in the constellation Taurus.
Unfortunately, there is no data at the moment as to it's size, probably because of the amount of stellar material still orbiting it.
One example of a T Tauri star is the T Tauri system, after which the star types were name for.
The dividing line is usually considered to be when the accretion process stops and the T tauri wind begins. This is probably approximately coincident with the beginning of lithium fusion (a T tauri star is not yet hot and dense enough for hydrogen fusion to start).
A protostar will live as long as 100,000 years. After material stops falling on the protostar it will enter then T Tauri star phase.
No. R136a1 is in the Tarantula Nebula, in the Large Magellanic Cloud, in the constellation Dorado
Aldebaran, aka Alpha Tauri, is in the constellation of Taurus which is one of the zodiac constellations.
One example of a T Tauri star is the T Tauri system, after which the star types were name for.
No, the T Tauri star is not a giant star, in fact it is a medium-sized star. It is also a very cold star.
T-Tauri phasee
Lawrence E. Cram has written: 'FGK stars and T Tauri stars' -- subject(s): Cool stars, T Tauri stars
No, all T Tauri stars are very young, only a million or so years old (it is a stage in the birth of a star). Thus the Sun was once a T Tauri star but as it is now 4600 million years old, it left that stage of its life a long time ago.
T Tauri stars are pre-main sequence stars. They are not a particular star and can vary in size depending on the propagator star and the amount of matter around it. For the individual star [See related question]
During its T-Tauri phase, when the Sun first started shining, it was not very bright. But it was very powerful, nevertheless, and spit out a stream of particles into space.
A T Tauri star is sort of a precursor of a star, or about to become a "real" star. Therefore, it can last anywhere from a few million to several trillion years before it runs out of energy, depending on its mass.
The dividing line is usually considered to be when the accretion process stops and the T tauri wind begins. This is probably approximately coincident with the beginning of lithium fusion (a T tauri star is not yet hot and dense enough for hydrogen fusion to start).
Yes. Zeta Tauri, Kappa Tauri, and Lambda Tauri are eclipsing binary stars.
Tauri Tiido goes by Tiido.
Epsilon Tauri b was created in 2007.