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Abstract:

Context. One of the most striking discoveries of the INTEGRAL observatory is the existence of a previously unknown population of X-ray sources in the inner arms of the Galaxy. The investigations of the optical/NIR counterparts of some of them have provided evidence that they are highly absorbed high mass X-ray binaries hosting supergiants. Aims. We aim to identify the optical/NIR counterpart of one of the newly discovered INTEGRAL sources, IGR J16283-4838, and determine the nature of this system. Methods. We present optical and NIR observations of the field of IGR J16283-4838, and use the astrometry and photometry of the sources within it to identify its counterpart. We obtain its NIR spectrum, and its optical/NIR spectral energy distribution by means of broadband photometry. We search for the intrinsic polarization of its light, and its short and long-term photometric variability. Results. We demonstrate that this source is a highly absorbed HMXB located beyond the Galactic center, and that it may be surrounded by a variable circumstellar medium. © 2010 ESO.

Registro:

Documento: Artículo
Título:Unveiling the nature of IGR J16283-4838
Autor:Pellizza, L.J.; Chaty, S.; Chisari, N.E.
Filiación:Instituto de Astronomía y Física Del Espacio, C.C. 67, Suc. 28, (1428) Buenos Aires, Argentina
Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET), Argentina
Laboratoire AIM, UMR 7158 CEA, Université Paris Diderot, 91191 Gif-sur-Yvette Cedex, France
Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08544, United States
Palabras clave:X-rays: binaries; X-rays: individuals: IGR J16283-4838; Circumstellar; Galactic Center; INTEGRAL observatory; Integral sources; NIR spectrum; Spectral energy distribution; X ray binaries; X-ray sources; X-rays: Binaries; X-rays: individual; Infrared devices; Photometers; Photometry; Spectroscopy; X ray optics; X rays
Año:2010
Volumen:526
Número:2
DOI: http://dx.doi.org/10.1051/0004-6361/201014954
Título revista:Astronomy and Astrophysics
Título revista abreviado:Astron. Astrophys.
ISSN:00046361
CODEN:AAEJA
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v526_n2_p_Pellizza

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Citas:

---------- APA ----------
Pellizza, L.J., Chaty, S. & Chisari, N.E. (2010) . Unveiling the nature of IGR J16283-4838. Astronomy and Astrophysics, 526(2).
http://dx.doi.org/10.1051/0004-6361/201014954
---------- CHICAGO ----------
Pellizza, L.J., Chaty, S., Chisari, N.E. "Unveiling the nature of IGR J16283-4838" . Astronomy and Astrophysics 526, no. 2 (2010).
http://dx.doi.org/10.1051/0004-6361/201014954
---------- MLA ----------
Pellizza, L.J., Chaty, S., Chisari, N.E. "Unveiling the nature of IGR J16283-4838" . Astronomy and Astrophysics, vol. 526, no. 2, 2010.
http://dx.doi.org/10.1051/0004-6361/201014954
---------- VANCOUVER ----------
Pellizza, L.J., Chaty, S., Chisari, N.E. Unveiling the nature of IGR J16283-4838. Astron. Astrophys. 2010;526(2).
http://dx.doi.org/10.1051/0004-6361/201014954