4.6 Article

Unveiling the nature of INTEGRAL objects through optical spectroscopy -: II.: The nature of four unidentified sources

Journal

ASTRONOMY & ASTROPHYSICS
Volume 448, Issue 2, Pages 547-556

Publisher

EDP SCIENCES S A
DOI: 10.1051/0004-6361:20054086

Keywords

X-rays : galaxies; X-rays : binaries; X-rays : individuals : IGR J12391-1610 (LEDA 170194); IGR J18406-0539 (SS 406); 2E 1853.7+1534; IGR J19473+4452

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We present new results from our optical spectrophotometric campaign ongoing at the Astronomical Observatory of Bologna in Loiano (Italy) on hard X-ray sources detected by INTEGRAL. We have observed spectroscopically the putative optical counterparts of four more INTEGRAL sources, IGR J12391- 1610, IGR J18406- 0539, 2E 1853.7+ 1534 and IGR J19473+ 4452. These data have allowed us to determine their nature, finding that IGR J12391- 1610 (= LEDA 170194) and IGR J19473+ 4452 are Seyfert 2 galaxies at redshifts z = 0.036 and z = 0.053, respectively, IGR J18406- 0539 (= SS 406) is a Be massive X-ray binary located at similar to 1.1 kpc from Earth, and 2E 1853.7+ 1534 is a type 1 Seyfert galaxy with z = 0.084. Physical parameters for these objects are also evaluated by collecting and discussing the available multiwavelength information. The determination of the extragalactic nature of a substantial fraction of sources inside the INTEGRAL surveys underlines the importance of hard X-ray observations for the study of background Active Galactic Nuclei located beyond the Zone of Avoidance of the Galactic Plane.

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