The turbulent past of the Milky Way's black hole

May 28, 2010
XMM-Newton images of the emission of the neutral iron fluorescent line in the molecular clouds around Sgr A* (Bridge, MC1 et MC2) between 2004 and 2008. The progression of the emission in the sub-regions indicated by ellipses 1,2, 3, and 4 of The Bridge are clearly shown. The distance traveled by the emission is 15 light years in less than 5 years. The angular scale (2 arc-minutes = 15 light years at the distance of the galactic center) and the direction towards Sgr A* are also shown. (c) Ponti G., et al., 2010, The Astrophysical Journal, V. 714, p. 732-747

The supermassive black hole at the center of our Galaxy went through turbulent times over the past centuries. We know this thanks to its surrounding molecular clouds, whose varying X-ray and gamma-ray luminosity reflects a major flare in the past. These findings, obtained by an international team of researchers led by French astrophysicists, are published in The Astrophysical Journal.

The located in usually show intense activity. But this is not true of our own Galaxy's black hole, Sgr A*, which shows very low activity. However, an international team of researchers, led by astrophysicists from the Astroparticle and Laboratory in Paris, has succeeded in showing that the black hole was active in the very recent past, and that it is therefore not as unusual as it seemed.

XMM-Newton and INTEGRAL, two ESA satellites to which CNES, CEA and CNRS-INSU have made a major contribution, have enabled researchers to observe X-ray and gamma-ray emissions from in the region of the galactic center, near Sgr A*. The scientists were surprised to discover that the emissions showed spectacular variation, such as the progressive brightening of one of the clouds between 2004 and 2009, at an apparent speed three times greater than that of light (see Fig. 1).

The phenomenon shows that the clouds reflect the high-energy radiation produced by the intense activity of the supermassive black hole. The light echo that reaches us is delayed in comparison with the direct light from the black hole. This delay depends on the position of the cloud and on the time the radiation takes to travel the distance from the black hole to the cloud. By observing the decay of the gamma-ray emission from another cloud (Fig. 2), the researchers estimated the duration and intensity of the flare, which began around four centuries ago and ended at the beginning of the twentieth century. For three hundred years, our Galaxy's supermassive black hole was therefore a million times brighter than now.

Explore further: Galaxy clusters collide—dark matter still a mystery

More information: ArXiv paper:

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5 / 5 (1) May 28, 2010
Might these observations of a x-ray light echo from Sag A* provide a similar explanation for the x-ray brightening seen in M 31*? [http://www.physor...880.html ] It seems possible that a previous outburst of M 31* is only now (post Jan 2006) illuminating a nearby cloud.

That story opines "The overall brightening since 2006 could be caused by M31* capturing winds from an orbiting star, or by a gas cloud that spiraled into the black hole. The increase in the rate of material falling towards the black hole is thought to drive an X-ray brightening of a relativistic jet." but also notes "We have some ideas about what's happening right around the black hole in Andromeda, but the truth is we still don't really know the details," Curious.
not rated yet May 31, 2010
Just a thing that bothers me... "at an apparent speed three times greater than that of light (see Fig. 1)".
First, nothing that we know of can be faster than the speed of light (gossip not taken into account). So how can it appear to be faster?
5 / 5 (1) May 31, 2010
These apparent superluminal speeds are an illusion caused by the geometry of the expanding light echo. The speed of light remains a constant and no laws are broken. Check out 'light echo': http://en.wikiped...ght_echo
not rated yet Jun 09, 2010
Hi yyz,
thanks for the clarification.
Although I have read the link, it is still a bit fuzy to me. However, the general idea is clear.

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