Details

Autor(en) / Beteiligte

• Ponti, G
• Jin, C
• De Marco, B
• Rea, N
• Rau, A
• Haberl, F
• Coti Zelati, F
• Bozzo, E
• Ferrigno, C
• Bower, G. C
• Demorest, P

Titel

Swift J174540.7−290015: a new accreting binary in the Galactic Centre

Ist Teil von

• Monthly notices of the Royal Astronomical Society, 2016-09, Vol.461 (3), p.2688-2701

Ort / Verlag

London: Oxford University Press

Erscheinungsjahr

2016

Link zum Volltext

Quelle

Alma/SFX Local Collection

Beschreibungen/Notizen

• We report on the identification of the new Galactic Centre (GC) transient Swift J174540.7−290015 as a likely low-mass X-ray binary located at only 16 arcsec from Sgr A⋆. This transient was detected on 2016 February 6, during the Swift GC monitoring, and it showed long-term spectral variations compatible with a hard- to soft-state transition. We observed the field with XMM–Newton on February 26 for 35 ks, detecting the source in the soft state, characterized by a low level of variability and a soft X-ray thermal spectrum with a high energy tail (detected by INTEGRAL up to ∼50 keV), typical of either accreting neutron stars or black holes. We observed: (i) a high column density of neutral absorbing material, suggesting that Swift J174540.7−290015 is located near or beyond the GC and; (ii) a sub-Solar iron abundance, therefore we argue that iron is depleted into dust grains. The lack of detection of Fe K absorption lines, eclipses or dipping suggests that the accretion disc is observed at a low inclination angle. Radio (Very Large Array) observations did not detect any radio counterpart to Swift J174540.7−290015. No evidence for X-ray or radio periodicity is found. The location of the transient was observed also in the near-infrared (near-IR) with gamma-ray burst optical near-IR detector at MPG/European Southern Observatory La Silla 2.2 m telescope and VLT/NaCo pre- and post-outburst. Within the Chandra error region, we find multiple objects that display no significant variations.