Open AccessA polarized infrared flare from Sagittarius A* and the signatures of orbiting plasma hotspots ★
Author(s) -
Trippe S.,
Paumard T.,
Ott T.,
Gillessen S.,
Eisenhauer F.,
Martins F.,
Genzel R.
Publication year - 2007
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1111/j.1365-2966.2006.11338.x
Subject(s) - physics , astrophysics , flare , supermassive black hole , astronomy , sagittarius a* , polarization (electrochemistry) , galaxy , position angle , infrared , chemistry
ABSTRACT In this article we summarize and discuss the infrared, radio and X‐ray emission from the supermassive black hole in the Galactic Centre, SgrA*. We include new results from near‐infrared polarimetric imaging observations obtained on 2006 May 31. In that night, a strong flare in K s band (2.08 μm) reaching top fluxes of ∼16 mJy could be observed. This flare was highly polarized (up to ∼40 per cent) and showed clear substructure on a time‐scale of 15 min, including a swing in the polarization angle of about 70°. For the first time we were able to observe both polarized flux and short‐time variability, with high significance in the same flare event. This result adds decisive information to the puzzle of the SgrA* activity. The observed polarization angle during the flare peak is the same as observed in two events in 2004 and 2005. Our observations strongly support the dynamical emission model of a decaying plasma hotspot orbiting SgrA* on a relativistic orbit. The observed polarization parameters and their variability with time might allow to constrain the orientation of accretion disc and spin axis with respect to the Galaxy.