Millimeter to X-ray flares from Sagittarius A*

0371579 - ASÚ 2013 RIV FR eng J - Článek v odborném periodiku
Eckart, A. - García-Marín, M. - Vogel, S. N. - Teuben, P. - Morris, M. - Baganoff, F. K. - Dexter, J. - Schoedel, R. - Witzel, G. - Valencia-S, M. - Karas, Vladimír - Kunneriath, Devaky - Straubmeier, C. - Moser, L. - Sabha, N. - Buchholz, R. M. - Zamaninasab, M. - Muzic, K. - Moultaka, J. - Zensus, J. A.
Millimeter to X-ray flares from Sagittarius A*.
Astronomy & Astrophysics. Roč. 537, January (2012), A52/1-A52/18. ISSN 0004-6361. E-ISSN 1432-0746
Grant ostatní: ESA(XE) ESA-PECS project No. 98040
Výzkumný záměr: CEZ:AV0Z10030501
Klíčová slova: galactic Centre * black holes
Kód oboru RIV: BN - Astronomie a nebeská mechanika, astrofyzika
Impakt faktor: 5.084, rok: 2012

We study the applicability of the adiabatic synchrotron source expansion model and study physical processes giving rise to the variable emission of SgrA* from the radio to the X-ray domain. Our observations were carried out on 18 May 2009 using the NACO adaptive optics (AO) instrument at the European Southern Observatory's Very Large Telescope, the ACIS-I instrument aboard the Chandra X-ray Observatory, the LABOCA bolometer at the Atacama Pathfinder EXperiment (APEX), and the CARMA mm telescope array at Cedar Flat, California.
Trvalý link: http://hdl.handle.net/11104/0205062