On the nature of the hard X-ray sources SWIFT J1907.3-2050, IGR J12123-5802 and IGR J19552+0044

The <i>INTEGRAL</i> and <i>Swift</i> hard X-ray surveys have identified a large number of new sources, among which many are proposed as Cataclysmic Variables (CVs). Here, we present the first detailed study of three X-ray-selected CVs, Swift J1907.3-2050, IGR J12123-5802 and...

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Autores principales: Bernardini, Federico, Martino, D. de, Mukai, K., Falanga, Maurizio, Andruchow, Ileana, Bonnet Bidaud, J. M., Masetti, N., Gonzalez Buitrago, D. H., Mouchet, M., Tovmassian, Gagik
Formato: Articulo
Lenguaje:Inglés
Publicado: 2013
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/85382
Aporte de:
id I19-R120-10915-85382
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Ciencias Astronómicas
X-rays: individual: IGR J19552+0044
X-rays: individual: Swift J1212.3-5806 (also known as: IGR J12123-5802 and 1RXS J121222.7-580118)
X-rays: individual: Swift J1907.3-2050 (also known as: V1082 Sgr)
X-rays: individual: WISE J195512.47+004536.6
spellingShingle Ciencias Astronómicas
X-rays: individual: IGR J19552+0044
X-rays: individual: Swift J1212.3-5806 (also known as: IGR J12123-5802 and 1RXS J121222.7-580118)
X-rays: individual: Swift J1907.3-2050 (also known as: V1082 Sgr)
X-rays: individual: WISE J195512.47+004536.6
Bernardini, Federico
Martino, D. de
Mukai, K.
Falanga, Maurizio
Andruchow, Ileana
Bonnet Bidaud, J. M.
Masetti, N.
Gonzalez Buitrago, D. H.
Mouchet, M.
Tovmassian, Gagik
On the nature of the hard X-ray sources SWIFT J1907.3-2050, IGR J12123-5802 and IGR J19552+0044
topic_facet Ciencias Astronómicas
X-rays: individual: IGR J19552+0044
X-rays: individual: Swift J1212.3-5806 (also known as: IGR J12123-5802 and 1RXS J121222.7-580118)
X-rays: individual: Swift J1907.3-2050 (also known as: V1082 Sgr)
X-rays: individual: WISE J195512.47+004536.6
description The <i>INTEGRAL</i> and <i>Swift</i> hard X-ray surveys have identified a large number of new sources, among which many are proposed as Cataclysmic Variables (CVs). Here, we present the first detailed study of three X-ray-selected CVs, Swift J1907.3-2050, IGR J12123-5802 and IGR J19552+0044 based on <i>XMM-Newton</i>, <i>Suzaku</i>, <i>Swift</i> observations and groundbased optical and archival (near-IR) nIR/IR data. Swift J1907.3-2050 is highly variable from hours to months-years at all wavelengths. No coherent X-ray pulses are detected but rather transient features. The X-ray spectrum reveals a multitemperature optically thin plasma absorbed by complex neutral material and a soft blackbody component arising from a small area. These characteristics are remarkably similar to those observed inmagnetic CVs. A suprasolar abundance of nitrogen could arise from nuclear processed material from the donor star. Swift J1907.3-2050 could be a peculiar magnetic CV with the second longest (20.82 h) binary period. IGR J12123-5802 is variable in the X-rays on a time-scale of ≳ 7.6 h. No coherent pulsations are detected, but its spectral characteristics suggest that it could be a magnetic CV of the Intermediate Polar (IP) type. IGR J19552+0044 shows two X-ray periods, ~1.38 h and ~1.69 h and an X-ray spectrum characterized by a multitemperature plasma with little absorption. We derive a low accretion rate, consistent with a CV below the orbital period gap. Its peculiar nIR/IR spectrum suggests a contribution from cyclotron emission. It could either be a pre-polar or an IP with the lowest degree of asynchronism.
format Articulo
Articulo
author Bernardini, Federico
Martino, D. de
Mukai, K.
Falanga, Maurizio
Andruchow, Ileana
Bonnet Bidaud, J. M.
Masetti, N.
Gonzalez Buitrago, D. H.
Mouchet, M.
Tovmassian, Gagik
author_facet Bernardini, Federico
Martino, D. de
Mukai, K.
Falanga, Maurizio
Andruchow, Ileana
Bonnet Bidaud, J. M.
Masetti, N.
Gonzalez Buitrago, D. H.
Mouchet, M.
Tovmassian, Gagik
author_sort Bernardini, Federico
title On the nature of the hard X-ray sources SWIFT J1907.3-2050, IGR J12123-5802 and IGR J19552+0044
title_short On the nature of the hard X-ray sources SWIFT J1907.3-2050, IGR J12123-5802 and IGR J19552+0044
title_full On the nature of the hard X-ray sources SWIFT J1907.3-2050, IGR J12123-5802 and IGR J19552+0044
title_fullStr On the nature of the hard X-ray sources SWIFT J1907.3-2050, IGR J12123-5802 and IGR J19552+0044
title_full_unstemmed On the nature of the hard X-ray sources SWIFT J1907.3-2050, IGR J12123-5802 and IGR J19552+0044
title_sort on the nature of the hard x-ray sources swift j1907.3-2050, igr j12123-5802 and igr j19552+0044
publishDate 2013
url http://sedici.unlp.edu.ar/handle/10915/85382
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