A&A 493, 119-125 (2009)
Mid-infrared VISIR and Spitzer observations of the surroundings of the magnetar SGR 1806-20F. Rahoui1, 2, S. Chaty1, and P.-O. Lagage1
1 Laboratoire AIM, CEA/DSM – CNRS – Université Paris Diderot, IRFU/Service d'Astrophysique, Bât. 709, CEA-Saclay, 91191 Gif-sur-Yvette Cedex, France
2 European Southern Observatory, Alonso de Córdova 3107, Vitacura, Santiago de Chile
Received 8 May 2008 / Accepted 23 October 2008
Context. SGR 1806-20 is the soft gamma-ray repeater that has exhibited the highest activity since its discovery, including a giant flare in 2004 December 27. Previous studies of this source – probably a magnetar – have shown that it was associated with a massive star cluster embedded in a gas and dust cloud. Moreover, several stars in the cluster are peculiar hypergiants – luminous blue variable (LBV) and Wolf-Rayet stars – exhibiting strong and likely dusty stellar winds.
Aims. We aimed at studying the mid-infrared emission of the stars associated with the same cluster as SGR 1806-20, to detect variations that could be due to the high-energy activity of the magnetar through interaction with the dust. We also studied the morphology of the cloud close to the centre of the cluster.
Methods. We carried out mid-infrared observations of SGR 1806-20 and its environment, with the highest spatial resolution in this domain to date, using ESO/VISIR in 2005 and 2006, and we retrieved Spitzer/IRAC-MIPS archival data of the same field. We performed broadband photometry of three stars – LBV 1806-20, a WC9 and an O/B supergiant – on our VISIR images, as well as on the IRAC data. We then built and fitted their broadband spectral energy distributions with a combination of two absorbed black bodies, representing their stellar components, as well as a possible mid-infrared excess, to derive their physical parameters.
Results. We show that LBV 1806-20 and the WC9 star exhibit a mid-infrared excess, likely because of the presence of circumstellar dust related to their winds. We also show that only LBV 1806-20 has had a variable flux over a period of two years, variability that is due to its LBV nature rather than to a heating of the gas and dust cloud by the high-energy emission of SGR 1806-20. Finally, differences in the intrinsic absorptions of the three stars show an inhomogeneous structure of the density of the gas and dust cloud in the massive star cluster.
Key words: stars: neutron -- infrared: stars -- dust, extinction -- open clusters and associations: general -- stars: early-type -- supergiants
© ESO 2008