Details

Autor(en) / Beteiligte

• 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.

Titel

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

Ist Teil von

• Monthly notices of the Royal Astronomical Society, 2013-11, Vol.435 (4), p.2822-2834

Ort / Verlag

London: Oxford University Press

Erscheinungsjahr

2013

Quelle

Alma/SFX Local Collection

Beschreibungen/Notizen

• 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.