The Center of Our Galaxy: Activity and High-Energy Emission of the Closest Massive Black Hole

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Invited paper at the 4th INTEGRAL Workshop, 4-8 September 2000, Alicante (Spain). To be published in the ESA-SP serie : 8 page

Scientific paper

The Center of our Galaxy is a peculiar region where a number of crucial astrophysical phenomena take place, from star formation to SN explosions and accretion onto a massive black hole. The quest for a massive black hole in the Galactic Nucleus is of course of particular relevance because, it would be the closest of such extreme objects, which are now believed to reside in most of the galactic nuclei of the universe. I will review here the main observational characteristics of the Galactic Center with particular attention to the the problem of existence, physical condition and activity of the 3 10E6 Mo black hole coincident with the compact radio source Sgr A*. I will report historical and recent results of high energy observations of the central degree of our Galaxy, along with the specific accretion models proposed to account for the apparent lack of high energy activity from Sgr A*. The scientific perspectives of the next X and gamma-ray missions in the domain of the Galactic Center physics are also mentioned.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

The Center of Our Galaxy: Activity and High-Energy Emission of the Closest Massive Black Hole does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The Center of Our Galaxy: Activity and High-Energy Emission of the Closest Massive Black Hole, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Center of Our Galaxy: Activity and High-Energy Emission of the Closest Massive Black Hole will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-726475

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.