VizieR Online Data Catalog: Multiwavelength study of Sgr A* (Mossoux+, 2016)
Abstract
Sgr A* is closest supermassive black hole is known to have a luminosity several orders of magnitude lower than the Eddington luminosity. Flares coming from the Sgr A* environment can be observed in infrared, X-ray, and submillimeter wavelengths, but their origins are still debated. We studied the X-ray, infrared, and radio flaring activity of Sgr A* close to the time of the Dusty S-cluster Object (DSO)/G2 pericenter passage in order to constrain the physical properties and origin of the flares. Simultaneous observations were made with XMM-Newton and WFC3 onboard HST during the period Feb-Apr 2014, in addition to coordinated observations with SINFONI at ESO's VLT, VLA in its A-configuration, and CARMA.
(5 data files).- Publication:
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VizieR Online Data Catalog
- Pub Date:
- March 2016
- DOI:
- 10.26093/cds/vizier.35890116
- Bibcode:
- 2016yCat..35890116M
- Keywords:
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- Milky Way;
- X-ray sources