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

• Published in: Monthly notices of the Royal Astronomical Society Vol. 435; no. 4; pp. 2822 - 2834
• Main Authors: Bernardini, F., de Martino, D., Mukai, K., Falanga, M., Andruchow, I., Bonnet-Bidaud, J.-M., Masetti, N., Buitrago, D. H. Gonzalez, Mouchet, M., Tovmassian, G.
• Format: Journal Article
• Language: English
• Published: London Oxford University Press 11.11.2013; Oxford University Press (OUP): Policy P - Oxford Open Option A
• Subjects: Astrophysics; Plasma; Pulsars; Sciences of the Universe; Star & galaxy formation; X-ray astronomy; X-rays: individual: IGR J19552+0044; X-rays: individual: Swift J1907.3−2050 (also known as: V1082 Sgr); X-rays: individual: Swift J1212.3−5806 (also known as: IGR J12123−5802 and 1RXS J121222.7−580118); X-rays: individual: WISE J195512.47+004536.6; X-rays: individual: Swift J1907.3-2050 (also known as: V1082 Sgr); X-rays: individual: Swift J1212.3-5806 (also known as: IGR J12123-5802 and 1RXS J121222.7-580118)
• ISSN: 0035-8711; 1365-2966
• DOI: 10.1093/mnras/stt1434

The INTEGRAL and Swift 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 XMM-Newton, Suzaku, Swift observations and ground-based 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 in magnetic CVs. A supra-solar 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.