HLX-1 brightest ultra-luminous X-ray source known.

[Philosophaie]

The most extreme ultra-luminous X-ray source, HLX-1 is 300light years from Earth. HLX-1 is the brightest ultra-luminous X-ray source known. Also it is not a supermassive black hole but it is the center of the galaxy. How can it be the brightest x-ray source and be a small black hole?

 

[turbo]

Luminosity falls off as the square of the distance from the emitter and the observer. Close enough, and any strong X-ray source (no matter how small) could be the "brightest".

 

[phyzguy]

Note that it is not 300 light years away, but 300 MILLION light years away. Slightly further.

 

[D H]

HLX-1 is the brightest ultra-luminous X-ray source known. Also it is not a supermassive black hole but it is the center of the galaxy. How can it be the brightest x-ray source and be a small black hole?

HLX-1 is in the galaxy ESO 243-49, about 300 million light years from the Earth. It is not at the center of a galaxy; that is one of the hallmarks of an ultraluminous X-ray source. The other hallmark is that they are ultraluminous, which means that their X-ray output exceeds that which would result from a stellar black hole.

In other words, ultraluminous X-ray sources are neither stellar-mass black holes nor active galactic nuclei. They are something in between, such as an intermediate mass black hole.

 

[sardar]

I find this discovery of HLX-1 to be quite intriguing. The fact that it is the brightest ultra-luminous X-ray source known despite not being a supermassive black hole is quite remarkable. This suggests that there may be other mechanisms at play in producing such intense X-ray emissions.

One possibility could be that HLX-1 is a stellar-mass black hole, but it is in a binary system with a high-mass companion star. This companion star could be transferring mass onto the black hole, causing it to emit large amounts of X-rays. Another explanation could be that HLX-1 has a powerful accretion disk, which is a disk of gas and dust that surrounds a black hole and produces intense X-ray emissions as matter falls into it.

Furthermore, the distance of 300 light years from Earth is also noteworthy. This puts HLX-1 relatively close to us in astronomical terms, making it an ideal target for further study and observation. By studying HLX-1, we may be able to gain a better understanding of the processes that drive such extreme X-ray emissions and how they relate to the center of a galaxy.

In conclusion, the discovery of HLX-1 challenges our current understanding of ultra-luminous X-ray sources and the role of black holes in producing such intense emissions. Further research and observations of HLX-1 will undoubtedly shed new light on this intriguing phenomenon.