Modeling mm- to X-ray flare emission from sagittarius A

Astronomy and Astrophysics

Volumn 500, Issue 3, 2009, Pages 935-946

  Eckart, A ^a,b   Baganoff, F K ^c   Morris, M R ^d   Kunneriath, D ^a,b   Zamaninasab, M ^a,b   Witzel, G ^a   Schodel R ^e   Garcia Marin M ^a   Meyer, L ^d   Bower, G C ^f   Marrone, D ^g   Bautz, M W ^c   Brandt, W N ^h   Garmire, G P ^h   Ricker, G R ^c   Straubmeier, C ^a   Roberts, D A ⁱ   Muzic, K ^a,b   Mauerhan, J ^d   Zensus, A ^a,b  

^a UNIVERSITY OF COLOGNE   (Germany)

^b MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^c MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

^d UNIVERSITY OF CALIFORNIA   (United States)

^e INSTITUTO DE ASTROFÍSICA DE ANDALUCÍA CSIC   (Spain)

^f UNIVERSITY OF CALIFORNIA   (United States)

^g HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^h PENNSYLVANIA STATE UNIVERSITY   (United States)

ⁱ NORTHWESTERN UNIVERSITY   (United States)

Author keywords

Accretion, accretion disks; Black hole physics; Galaxy: center; Galaxy: nucleus; Infrared: general; X rays: general

Indexed keywords

ACCRETION, ACCRETION DISKS; BLACK HOLE PHYSICS; GALAXY: CENTER; GALAXY: NUCLEUS; INFRARED: GENERAL; X-RAYS: GENERAL;

BUILDINGS; DISKS (MACHINE COMPONENTS); DISKS (STRUCTURAL COMPONENTS); GALAXIES; LIGHT; MAGNETIC DOMAINS; MAGNETIC FIELDS; OBSERVATORIES; OPTICAL TELESCOPES; OPTICAL WAVEGUIDES; STARS;

X RAYS;

EID: 67650591064     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200811354     Document Type: Article

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