luminous blue variables oor Spaans
luminous blue variables
Vertalings in die woordeboek Engels - Spaans
Variable luminosa azul
en
class of variable stars; highly luminous blue pulsing super- or hypergiants
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Many of them become luminous blue variables (LBVs) with episodes of extreme mass loss.
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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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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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Shortly afterwards two emission line stars were classified as Wolf Rayet stars, and a third as a Luminous Blue Variable that was thought to be one of the most luminous stars in the galaxy.
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G10.3-0.1 is the most notable as it contains the star cluster 1806-20 that includes the famous Luminous Blue Variable star LBV 1806-20, the magnetar SGR 1806-20, two blue hypergiant stars, a supergiant O star, three Wolf-Rayet stars, two of them carbon-rich, and other young, massive stars.
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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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Luminous blue variables are very massive, unstable stars advanced in their evolution.
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a) 26 Luminous Blue Variables and Wolf Rayet star candidates, including R136a1.
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Many of them become luminous blue variables with episodes of extreme mass loss.
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Main article: Luminous blue variable
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Left: position of Luminous Blue Variable star (LBV) where explosion was detected in 2015. ON A FAST TRACK TO THE WOLF-RAYET PHASE
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In the current theoretical framework, luminous blue variables are massive stars in a transition to a Wolf-Rayet phase, which is supposed to be the last phase of its life.
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In this work, we present the results of the 2007 observing season of our long-term photometric monitoring campaign of Eta Carinae, the brightest Luminous Blue Variable in our galaxy.
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"Luminous blue variable stars like this one show two different kinds of eruptions: regular outbursts after which the star returns to its original state and giant eruptions which alter the star permanently.
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Observatory Eta Carinae This new image of the luminous blue variable Eta Carinae was taken with the NACO near-infrared adaptive optics instrument on ESO's Very Large Telescope, yielding an incredible amount of detail.
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IMAX movies Carinae This new image of the luminous blue variable Eta Carinae was taken with the NACO near-infrared adaptive optics instrument on ESO's Very Large Telescope, yielding an incredible amount of detail.
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Working with the ELT Carinae This new image of the luminous blue variable Eta Carinae was taken with the NACO near-infrared adaptive optics instrument on ESO's Very Large Telescope, yielding an incredible amount of detail.
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"Now we know already several cases of these luminous blue variables that follow the same pattern: smaller, more or less continuous eruption over several decades and an outburst between 40 and 80 days before the main explosion.
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The Luminous Blue Variables and Wolf Rayet star candidates, including R136a1. These are very massive sources, which are very short lived and formed very recently, so they trace the current episode in chemical evolution in the LMC as well as crucial information on the kinematics and properties of the massive clusters in which they form.
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a) 26 Luminous Blue Variables and Wolf Rayet star candidates, including R136a1. These are very massive sources, which are very short lived and formed very recently, so they trace the current episode in chemical evolution in the LMC as well as crucial information on the kinematics and properties of the massive clusters in which they form.
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But before they can enter this phase, they have to get rid of their outer envelope and the mechanism for that is still unknown: the stars can lose their envelope though very strong stellar winds, however, these winds might result being very inefficient to achieve the transition to the Wolf-Rayet phase; a single giant eruption does not seem to solve the problem either, as we see in Eta Carinae, which has already suffered at least two giant eruptions and still continues as a luminous blue variable star. Nevertheless, a violent eruption such as SN 2015bh could be a way to fast-track the star’s evolution to its last phase. If SN 2015bh and other events with similar pattern have survived this explosion, they could already be on their way to become Wolf-Rayet stars.
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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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22 sinne gevind in 13 ms. Hulle kom uit baie bronne en word nie nagegaan nie.