radiation Graceli cones progressively increase as the poles as the energy of the particle system, stars, galaxies and black holes.
This variation occurs as the temperature increases, or that variation can occur even fields or rotational dynamics.
a radiação Graceli dos cones dos polos aumentam progressivamente conforme conforme a energia do sistema de particulas, astros, galáxias e buracos negro.
esta variação acontece conforme a temperatura aumenta, ou mesmo que pode ocorrer variação de campos ou mesmo de dinâmica rotacional.
quinta-feira, 14 de novembro de 2013
Graceli radiation cones .
cones of black hole radiation occur in all galaxies flat , these cones ejection radiation also occur in stars and all stars, but also occur at the poles of all the particles of the least to the most massudas .
ie , the galaxies are also constituted of hemispheres and poles .
13 November 2013
Astronomers studying a black hole in our Galaxy with ESA’s XMM-Newton observatory have made a surprising discovery about the cocktail of particles that are ejected from its surroundings.
Stellar-mass black holes are often found feasting on material from a companion star. Matter flows from the star towards the black hole, circling in a disc around it with a temperature so high that it emits X-rays.
The black hole can be a fussy eater: instead of swallowing all of the material, it sometimes pushes a fraction of it away in the form of two powerful jets of particles. Because these jets release mass and energy into the surroundings, the black hole has less material to feed on.
By studying the composition of the jets, we can learn more about the feeding habits of black holes.
Observations at radio wavelengths have already found that black hole jets contain electrons moving at close to the speed of light. But, until now, it was not clear whether the negative charge of the electrons is complemented by their anti-particles, positrons, or rather by heavier positively-charged particles in the jets, like protons or atomic nuclei.
In a new study, astronomers have used XMM-Newton to study a black hole binary system called 4U1630–47, well known to show outbursts of X-rays over periods of months and years.
“In our observations, we found signs of highly ionised nuclei of two heavy elements, iron and nickel,” says María Díaz Trigo of the European Southern Observatory in Munich, Germany, lead author of the paper published in the journal Nature.
“The discovery came as a surprise – and a good one, since it shows beyond doubt that the composition of black hole jets is much richer than just electrons.”
The team of astronomers observed 4U1630–47 with XMM-Newton on two occasions in September 2012, and compared the results with near-simultaneous radio observations from the Australia Telescope Compact Array.
Although the two sets of observations described by Dr Díaz Trigo and collaborators were separated by only a couple of weeks, the results were surprisingly different.
In the first set of observations, the astronomers detected X-rays from the accretion disc, but did not see anything in radio waves – a sign that the jets were not active.
But in the second set, they detected the source both in X-rays and radio waves, so they knew the jets had been reactivated in the meantime.
CO
cones of black hole radiation occur in all galaxies flat , these cones ejection radiation also occur in stars and all stars, but also occur at the poles of all the particles of the least to the most massudas .
ie , the galaxies are also constituted of hemispheres and poles .
13 November 2013
Astronomers studying a black hole in our Galaxy with ESA’s XMM-Newton observatory have made a surprising discovery about the cocktail of particles that are ejected from its surroundings.
Stellar-mass black holes are often found feasting on material from a companion star. Matter flows from the star towards the black hole, circling in a disc around it with a temperature so high that it emits X-rays.
The black hole can be a fussy eater: instead of swallowing all of the material, it sometimes pushes a fraction of it away in the form of two powerful jets of particles. Because these jets release mass and energy into the surroundings, the black hole has less material to feed on.
By studying the composition of the jets, we can learn more about the feeding habits of black holes.
Observations at radio wavelengths have already found that black hole jets contain electrons moving at close to the speed of light. But, until now, it was not clear whether the negative charge of the electrons is complemented by their anti-particles, positrons, or rather by heavier positively-charged particles in the jets, like protons or atomic nuclei.
In a new study, astronomers have used XMM-Newton to study a black hole binary system called 4U1630–47, well known to show outbursts of X-rays over periods of months and years.
“In our observations, we found signs of highly ionised nuclei of two heavy elements, iron and nickel,” says María Díaz Trigo of the European Southern Observatory in Munich, Germany, lead author of the paper published in the journal Nature.
“The discovery came as a surprise – and a good one, since it shows beyond doubt that the composition of black hole jets is much richer than just electrons.”
The team of astronomers observed 4U1630–47 with XMM-Newton on two occasions in September 2012, and compared the results with near-simultaneous radio observations from the Australia Telescope Compact Array.
Although the two sets of observations described by Dr Díaz Trigo and collaborators were separated by only a couple of weeks, the results were surprisingly different.
In the first set of observations, the astronomers detected X-rays from the accretion disc, but did not see anything in radio waves – a sign that the jets were not active.
But in the second set, they detected the source both in X-rays and radio waves, so they knew the jets had been reactivated in the meantime.
CO
cones de radiação Graceli.
cones de radiação de buracos negros acontecem em todas as galáxias planas, estes cones de ejeção de radiação também acontecem nas estrelas e todos astros, mas também acontecem nos polos de todas as partículas das menos até as mais massudas.
ou seja, as galáxias também são constituídas de hemisférios e polos.
cones de radiação de buracos negros acontecem em todas as galáxias planas, estes cones de ejeção de radiação também acontecem nas estrelas e todos astros, mas também acontecem nos polos de todas as partículas das menos até as mais massudas.
ou seja, as galáxias também são constituídas de hemisférios e polos.
cones de radiação Graceli.
cones de radiação de buracos negros acontecem em todas as galáxias planas, estes cones de ejeção de radiação tambem acontecem nas estrelas e todos astros, mas tambem acontecem nos polos de todas as partículas das menos até as mais massudas.
ou seja, as galáxias também sao constituidas de hemisférios e polos.
cones de radiação de buracos negros acontecem em todas as galáxias planas, estes cones de ejeção de radiação tambem acontecem nas estrelas e todos astros, mas tambem acontecem nos polos de todas as partículas das menos até as mais massudas.
ou seja, as galáxias também sao constituidas de hemisférios e polos.
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