The Size, Shape, and Scattering of Sagittarius A* at 86 GHz: First VLBI with ALMA

18 Jan 2019S. IssaounM. D. JohnsonL. BlackburnC. D. BrinkerinkM. MościbrodzkaA. ChaelC. GoddiI. Martí-VidalJ. WagnerS. S. DoelemanH. FalckeT. P. KrichbaumK. AkiyamaU. BachK. L. BoumanG. C. BowerA. BroderickI. ChoG. CrewJ. DexterV. FishR. GoldJ. L. GómezK. HadaA. Hernández-GómezM. JanßenM. KinoM. KramerL. LoinardR. -S. LuS. MarkoffD. P. MarroneL. D. MatthewsJ. M. MoranC. MüllerF. RoelofsE. RosH. RottmannS. SanchezR. P. J. TilanusP. de VicenteM. WielgusJ. A. ZensusG. -Y. Zhao

The Galactic Center supermassive black hole Sagittarius A* (Sgr A*) is one of the most promising targets to study the dynamics of black hole accretion and outflow via direct imaging with very long baseline interferometry (VLBI). At 3.5 mm (86 GHz), the emission from Sgr A* is resolvable with the Global Millimeter VLBI Array (GMVA)... (read more)

PDF Abstract

Code


No code implementations yet. Submit your code now

Tasks


Results from the Paper


  Submit results from this paper to get state-of-the-art GitHub badges and help the community compare results to other papers.