luminous blue variables oor Portugees
luminous blue variables
Vertalings in die woordeboek Engels - Portugees
Variável luminosa azul
en
class of variable stars; highly luminous blue pulsing super- or hypergiants
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HR Carinae is a luminous blue variable star located in the constellation Carina.
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HR Carinae undergoes spectral variations apparently correlated with the light variations similarly to other luminous blue variables.
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The luminous blue variable Eta Carinae has recently been determined to be a binary star system.
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They are also known as Type V supernovae, Eta Carinae analogs, and giant eruptions of luminous blue variables (LBV).
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This star belongs to its own eponymous S Doradus class of variable stars, also designated as luminous blue variables or LBVs.
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A recent Hubble image provides further evidence that a star in our galaxy is a rare type of star called “a luminous blue variable.”
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Such a scenario might occur following mass loss of 10 or more M☉ in a luminous blue variable eruption, or through pulsational pair instability ejections.
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The Pistol Star, a luminous blue variable is 1.6 million times brighter than the Sun making it one of the most luminous stars in the Milky Way.
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It contains the Soft gamma repeater SGR 1806-20 and the luminous blue variable hypergiant LBV 1806-20, a candidate for the most luminous star in the Milky Way.
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Luminous blue variables (LBVs) were identified as likely candidates near the upper luminosity limit and showing this intense mass loss which strips away much of their outer layers of the star.
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It is expected that stars like UY Scuti should evolve back to hotter temperatures to become a yellow hypergiant, luminous blue variable, or a Wolf–Rayet star, creating a strong stellar wind that will eject its outer layers and expose the core, before exploding as a type IIb, IIn, or type Ib/Ic supernova.
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Key: O: O-type main-sequence star Of: evolved O-type showing N and He emission BSG: blue supergiant RSG: red supergiant YHG: yellow hypergiant LBV: luminous blue variable WNh: WN plus hydrogen lines WNL: "late" WN-class Wolf–Rayet star (about WN6 to WN9) WNE: "early" WN-class Wolf–Rayet star (about WN2 to WN6) WC: WC-class Wolf–Rayet star WO: WO-class Wolf–Rayet star Wolf–Rayet stars form from massive stars, although the evolved population I stars have lost half or more of their initial masses by the time they show a WR appearance.
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LBV: luminous blue variable
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SIMBAD data LBV 1806-20 is a candidate luminous blue variable (LBV) and likely binary star located nearly 40,000 light-years from the Sun, towards the center of the Milky Way.
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The luminous blue variable HD 168607, located in the south-east part of the Omega nebula, is generally assumed to be associated with it; its close neighbor, the blue hypergiant HD 168625, may be too.
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Some of these high-mass stars then spend just a few million years in the post-red supergiant phase as yellow hypergiants, a relatively short time in the life of a star, before rapidly evolving into another unusual type of star called a luminous blue variable.
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According to the classification by astrophysicists, it is ranked as a supergiant star of an extremely rare class of blue luminous variable stars, which currently has only a few tens of members but which must have been common in the early days of the Universe.
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