Volume 490, Number 2, November I 2008
|Page(s)||801 - 806|
|Published online||17 September 2008|
High-resolution X-ray spectroscopy of θ Carinae*
Institut d'Astrophysique et de Géophysique, Université de Liège, Allée du 6 août 17, Bât. B5C, 4000 Liège, Belgium e-mail: email@example.com
Accepted: 21 August 2008
Context. The peculiar hot star θ Car in the open cluster IC 2602 is a blue straggler as well as a single-line binary with a short period (2.2d).
Aims. Its high-energy properties are not well known, though X-rays can provide useful constraints on the energetic processes at work in binaries as well as in peculiar, single objects.
Methods. We present the analysis of a 50 ks exposure taken with the XMM-Newton observatory. It provides medium as well as high-resolution spectroscopy.
Results. Our high-resolution spectroscopy analysis reveals a very soft spectrum with multiple temperature components (1–6 MK) and an X-ray flux slightly below the `canonical' value . The X-ray lines appear surprisingly narrow and unshifted, reminiscent of those of β Cru and τ Sco. Their relative intensities confirm the anomalous abundances detected in the optical domain (C strongly depleted, N strongly enriched, O slightly depleted). In addition, the X-ray data favor a slight depletion in neon and iron, but they are less conclusive for the magnesium abundance, which may be solar-like. While no significant changes occur during the XMM-Newton observation, variability in the X-ray domain is detected in the long-term range. The formation radius of the X-ray emission is loosely constrained to < 5 , which allows for a range of models (wind-shock, corona, magnetic confinement, ...) though not all of them can be reconciled with the softness of the spectrum and the narrowness of the lines.
Key words: X-rays: stars / stars: individual: θ Carinae / stars: early-type
© ESO, 2008
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