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dc.contributor.authorEckart, Andreas-
dc.contributor.authorSchödel, Rainer-
dc.contributor.authorGarcía-Marín, Macarena-
dc.contributor.authorWitzel, Gunther-
dc.contributor.authorWeiss, Achim-
dc.contributor.authorBaganoff, Frederick Keith-
dc.contributor.authorMorris, Mark R.-
dc.contributor.authorBertram, Thomas-
dc.contributor.authorDovciak, Michal-
dc.contributor.authorDuschl, Wolfang J.-
dc.contributor.authorKaras, V.-
dc.contributor.authorKoenig, Stefan-
dc.contributor.authorKrichbaum, Thomas P.-
dc.contributor.authorKrips, Melanie-
dc.contributor.authorKunneriath, D.-
dc.contributor.authorLu, Rong S.-
dc.contributor.authorMarkoff, Sera-
dc.contributor.authorMauerhan, Jon Christian-
dc.contributor.authorMeyer, Laurence-
dc.contributor.authorMoultaka, Jihane-
dc.contributor.authorMuzic, Koraljka-
dc.contributor.authorNajarro, Francisco-
dc.contributor.authorPott, Jörg Uwe-
dc.contributor.authorSchuster, Karl F.-
dc.contributor.authorSjouwerman, Lorant O.-
dc.contributor.authorStraubmeier, Christian-
dc.contributor.authorThum, Clemens-
dc.contributor.authorVogel, Stuart N.-
dc.contributor.authorWiesemeyer, Helmut-
dc.contributor.authorZamaninasab, Mohammad-
dc.contributor.authorZensus, J. Antón-
dc.date.accessioned2008-11-19T08:26:50Z-
dc.date.available2008-11-19T08:26:50Z-
dc.date.issued2008-11-17-
dc.identifier.citationarXiv:0811.2753v1 [astro-ph]en_US
dc.identifier.urihttp://hdl.handle.net/10261/8664-
dc.description12 pages, 9 figures, 3 tables.-- In press with Astronomy & Astrophysics.en_US
dc.description.abstractWe report on a successful, simultaneous observation and modeling of the sub-millimeter to near-infrared flare emission of the Sgr A* counterpart associated with the super-massive black hole at the Galactic center. Our modeling is based on simultaneous observations that have been carried out on 03 June, 2008 using the NACO adaptive optics (AO) instrument at the ESO VLT and the LABOCA bolometer at the APEX telescope. Inspection and modeling of the light curves show that the sub-mm follows the NIR emission with a delay of 1.5+/-0.5 hours. We explain the flare emission delay by an adiabatic expansion of the source components.en_US
dc.description.sponsorshipWe are grateful to all the ESO PARANAL and Sequitor staff, and especially to the members of the NAOS/CONICA, VLTI, and APEX team. The observations were made possible through a special effort by the APEX/ONSALA staff to have the LABOCA bolometer ready for triggering. Leo Meyer is supported by the DAAD exchange program. Macarena García-Marín is supported by the German federal department for education and research (BMBF) under the project numbers: 50OS0502 & 50OS0801. The X-ray work was supported by NASA through Chandra award G05-6093X. M. Zamaninasab, D. Kunneriath, and R.-S. Lu, are members of the International Max Planck Research School (IMPRS) for Astronomy and Astrophysics at the MPIfR and the Universities of Bonn and Cologne. R. Schödel acknowledges support by the Ramón y Cajal programme by the Ministerio de Ciencia e Innovación of the government of Spain.en_US
dc.format.extent189209 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoengen_US
dc.relation.isversionofPreprint-
dc.rightsopenAccessen_US
dc.subjectBlack hole physicsen_US
dc.subjectInfrared: generalen_US
dc.subjectAccretionen_US
dc.subjectAccretion disksen_US
dc.subjectGalaxy: centeren_US
dc.subjectNucleusen_US
dc.subjectBlack Holes: individual: SgrA*en_US
dc.titleSimultaneous NIR/sub-mm observation of flare emission from SgrA*en_US
dc.typepreprinten_US
dc.description.peerreviewedPeer revieweden_US
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