pith. machine review for the scientific record. sign in

arxiv: 1008.1560 · v1 · submitted 2010-08-09 · 🌌 astro-ph.GA

Recognition: unknown

Coordinated NIR/mm observations of flare emission from Sagittarius A*

Authors on Pith no claims yet
classification 🌌 astro-ph.GA
keywords emissionflareassociatedblackcentrecontinuouscoordinatedcounterpart
0
0 comments X
read the original abstract

We report on a successful, simultaneous observation and modelling of the millimeter (mm) to near-infrared (NIR) flare emission of the Sgr A* counterpart associated with the supermassive black hole at the Galactic centre (GC). We present a mm/sub-mm light curve of Sgr A* with one of the highest quality continuous time coverages and study and model the physical processes giving rise to the variable emission of Sgr A*.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.