Solar Energy News  
Integral Sees The Galactic Centre Playing Hide And Seek

This mosaic image, built with exposures obtained by the IBIS/ISGRI instrument on board ESA's Integral gamma-ray observatory in April 2006, shows the Galactic centre region, an area of the sky supposed to host a gigantic black hole and characterised by the presence of a variety of hard X-ray and gamma-ray point sources. Due to the variability these sources possess on all time scales, the region never looks exactly the same.

Surprisingly, the sources were 'off' around the time of the observation (including the normally bright well-known black-hole candidate and micro-quasar 1E 1740.7-2942), displaying an unusually 'quiet' galactic centre. This is a very different view from those obtained on the long-term average. The sources and the positions marked in white are almost permanently visible, while those marked in red are known 'transient' sources, that is sources more often 'off' than 'on'.

The source called 1E 1740.7-2942 is normally the brightest source in the Galactic Centre region. It is a well-known black-hole candidate, as well as a micro-quasar source. The massive black hole at the very centre of our Galaxy, Sagittarius A* (or Sgr A*), is very close to source marked as '1', corresponding to IGR J17456-2901. The image covers a sky area of 4.3x2 degrees, and it is centred on (0, -0.5) degrees in Galactic coordinates. Credits: ESA/ISDC

by Staff Writers
Paris, France (ESA) Jan 19, 2007
ESA's gamma ray observatory Integral has caught the centre of our galaxy in a moment of rare quiet. A handful of the most energetic high-energy sources surrounding the black hole at the centre of the Galaxy had all faded into a temporary silence when Integral looked. This unusual event is allowing astronomers to probe for even fainter objects and may give them a glimpse of matter disappearing into the massive black hole at the centre of our galaxy.

The Galactic centre is one of the most dynamic places in our Galaxy. It is thought to be home to a gigantic black hole, called Sagittarius A* (pronounced 'A star'). Since the beginning of the Integral mission, ESA's gamma ray observatory has allowed astronomers to keep watch on this ever-changing environment.

Integral has discovered many new sources of high-energy radiation near the galactic centre. From February 2005, Integral began to regularly monitor the centre of the Galaxy, and its immediate environment, known as the Galactic bulge.

Erik Kuulkers of ESA's Integral Science Operations Centre, ESAC, Spain, leads the Galactic bulge monitoring programme. Integral now keeps its high-tech eyes on about 80 high-energy sources in the galactic bulge. "Most of these are X-ray binaries," says Kuulkers.

X-ray binaries are made up of two stars in orbit around one another. One star is a relatively normal star; the other is a collapsed star, such as a white dwarf, neutron star or even a black hole. If the stars are close enough together, the strong gravity of the collapsed star can pull off gaseous material from the normal star.

As this gas spirals down around the collapsed star, it is heated to over a million degrees centigrade and this causes it to emit high energy X-rays and gamma rays. The amount of gas falling from one star to the other determines the brightness of the X-ray and gamma-ray emission.

According to the Integral observations in April 2006, the high-energy rays from about ten sources closest to the galactic centre all faded temporarily. Kuulkers excludes the possibility that a mysterious external force is acting on all the objects to drive them into quiescence. "All the sources are variable and it was just by accident or sheer luck that they had turned off during that observation," he says with a smile.

The fortuitous dimming allows astronomers to set new limits on how faint these X-ray binaries can become. It also allows a number of new investigations to be undertaken with the data.

"When these normally bright sources are faint, we can look for even fainter sources," says Kuulkers. These could be other X-ray binaries or the high-energy radiation from giant molecular clouds interacting with past supernovae. There is also the possibility of detecting the faint high-energy radiation from the massive black hole in our Galaxy's centre.

Integral's Galactic bulge monitoring programme will continue throughout this year. The data is made available, within a day or two of being collected, to the scientific community via the Internet from a dedicated webpage at the Integral Science Data Centre (IDSC), Geneva, Switzerland. This way, anyone interested in specific sources can watch for interesting changes and trigger follow up observations with other telescopes in good time.

The findings are accepted for publication in the Astronomy and Astrophysics magazine, in the article titled: "The INTEGRAL Galactic bulge monitoring program: the first 1.5 years", by E.Kuulkers et al.

Related Links
ESA's gamma-ray astronomy mission
Stellar Chemistry, The Universe And All Within It
Stellar Chemistry, The Universe And All Within It



Memory Foam Mattress Review
Newsletters :: SpaceDaily :: SpaceWar :: TerraDaily :: Energy Daily
XML Feeds :: Space News :: Earth News :: War News :: Solar Energy News


Are North Korea Sanctions Working
Seoul (UPI) Jan 17, 2007
Are three-month-long international sanctions on North Korea effectively forcing the defiant country to finally give up its nuclear weapons program? The answer seems unclear for now as China and South Korea, North Korea's main economic lifelines, have stayed away from major sanctions against their neighbor for fear of possible turmoil in the region. With growing skepticism about the effectiveness of economic sanctions, North Korea has launched campaigns to endure outside pressure, saying it would focus national efforts on building a self-supporting economy.







  • Zapatero Pins Faith In Renewable Energy Amid Nuclear Debate
  • Nuclear Waste Land
  • Most Germans Oppose Nuclear Power Phase-Out
  • Czech Republic's Temelin Nuclear Reactor Back On Stream

  • Climate Change Could Amplify Drought In East Indian Ocean And Australasia
  • Evangelicals Embrace Climate Change Science To Save The World
  • Lloyd's Insurance Boss Demands Action On Climate Change
  • Nigerian President Calls For International Action On Climate Change

  • California Fruit Crops Devastated By Freeze Says Schwarzenegger
  • California's Big Freeze Threatening Citrus Crops
  • 150,000 Trout Killed At Fish Farm In Storm Off Norway
  • Clear Strong Guidelines Needed For Marine Aquaculture

  • Big Vegetarian Mammals Play Critical Role In Maintaining Healthy Ecosystems
  • Big-Brained Birds Survive Better
  • Scientists Discover New Life Forms In The Arctic Ocean
  • Largest Flower Evolved From Family Of Much Tinier Blooms

  • India To Conduct Full-Duration Cryogenic Stage Test
  • XCOR Aerospace Begins Test Firing Of Methane Rocket Engine
  • Research Continues For Deep Space Travel Propulsion
  • Gravity Mission To Benefit From QinetiQ Precision



  • Chairman Reacts to National Academies' Earth Science and Applications Assessment
  • Egypt Plans First Remote Sensing Satellite
  • Japanese Government Initiates Space-Borne Hyperspectral Payload Program
  • US Climate Satellites Imperiled By Low Federal Funding Say EO Scientists

  • LISA Pathfinder Spacecraft Test Phase About To Start
  • ESA On Target For Rosetta Mars Swing By February 25
  • LockMart Completes Tracking With Open Architecture And Solid-State Radar Antenna
  • University Of Chicago Receives Supercomputer Time For Supernova Simulations

  • The content herein, unless otherwise known to be public domain, are Copyright Space.TV Corporation. AFP and UPI Wire Stories are copyright Agence France-Presse and United Press International. ESA Portal Reports are copyright European Space Agency. All NASA sourced material is public domain. Additional copyrights may apply in whole or part to other bona fide parties. Advertising does not imply endorsement, agreement or approval of any opinions, statements or information provided by Space.TV Corp on any Web page published or hosted by Space.TV Corp. Privacy Statement