There are stars with spectral classes of O & B (e.g. Rigel) R136a1 is a star of the spectral class WN5h. Wolf Rayet stars have this kind of spectral type.
stars in spectral classes O, B, or A would be a bright bluish color, leaning towards a purplish color as you go from A to O.
The most massive main sequence stars are typically blue in color. These stars are classified as O-type stars, characterized by their high temperatures and luminosities. Their intense heat causes them to emit light primarily in the blue and ultraviolet spectrum. Examples include stars like Zeta Ophiuchi and the stars in the Pleiades cluster.
On the Hertzsprung-Russell (H-R) diagram, stars that have high temperature and high luminosity are typically found in the upper left quadrant, classified as O-type or B-type stars. These stars are massive and emit a significant amount of energy due to their high temperatures, often exceeding 30,000 Kelvin. They are characterized by their blue or blue-white colors and have relatively short lifespans compared to less massive stars.
T Tauri stars are pre-Main Sequence stars which are large but not as hot as O and B Main Sequence stars. They mainly fall in the categories of F, G, K or M, and they are not yet on the Main Sequence because they are still accreting mass and are still very young and unstable.
The main sequence stars on the Hertzsprung-Russell diagram that are least massive are the red dwarfs. These stars have low masses compared to other main sequence stars like our sun. They are cooler and fainter, making them difficult to observe compared to more massive stars.
O and B main sequence stars are rare because they are massive stars with short lifespans compared to smaller stars like the Sun. Their high mass causes them to burn through their nuclear fuel at a faster rate, leading to a shorter main sequence lifetime. This means that O and B stars are less common in the overall population of stars because they exist for a shorter period of time.
O. This is the class of the blue/white giants.
Massive, hot, and young stars are typically the brightest at ultraviolet wavelengths. These stars emit a large amount of ultraviolet radiation due to their high surface temperatures, making them stand out in the ultraviolet spectrum. Examples include O-type and B-type stars.
The most massive main sequence stars are typically blue in color, due to their high surface temperatures. These stars are known as O-type stars and can be tens of times more massive than the Sun.
The correct classification for the stars is O,B,A,F,G,M,K.
3 stars in orians belt
O, B, A, F, G, K, and M
The massive stars turn into gas
Some massive stars will become neutron stars. When massive stars die they will either become neutron stars or black holes depending on how much mass is left behind.
stars in spectral classes O, B, or A would be a bright bluish color, leaning towards a purplish color as you go from A to O.
Main sequence stars that are most massive are O-type stars, which can be more than 16 times the mass of the Sun. These stars are among the hottest and brightest in the main sequence and have relatively short lifespans compared to lower mass stars.
O, B, A, F, G, K, and M.