The broad band spectral properties of SgrA* . The fate of the dusty object approaching the center

0423356 - ASÚ 2014 RIV IT eng J - Journal Article
Eckart, A. - Muzic, K. - Yazici, S. - Sabha, N. - Shahzamanian, B. - Witzel, G. - Moser, L. - García-Marín, M. - Valencia-S, M. - Jalali, B. - Bremer, M. - Straubmeier, C. - Rauch, C. - Buchholz, R. M. - Kunneriath, Devaky - Moultaka, J.
The broad band spectral properties of SgrA* . The fate of the dusty object approaching the center.
Memorie della Societa Astronomica Italiana. Roč. 84, č. 3 (2013), s. 618-621. ISSN 0037-8720.
[X-ray astronomy: towards the next 50 years! Milano, 01.10.2012-05.10.2012]
Institutional support: RVO:67985815
Keywords : galaxy center * infrared stars
Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics

The super-massive 4 million solar mass black hole (SMBH) SgrA* shows flare emission from the millimeter to the X-ray domain. A flare analysis in the framework of a Synchrotron Self Compton (SSC) mechanism shows that a scenario in which the infrared flares are explained by synchrotron emission and the associated X-ray flares are produced via SSC emission can also explain the variability spectrum observed in the sub-millimeter radio domain. In September 2013 a dust object will pass by SgrA* giving hope for extraordinary flare events that will tell us more about the accretion and radiation mechanism close to the super massive black hole.
Permanent Link: http://hdl.handle.net/11104/0229453