2007/12/04 by A. J. J. Raassen, K. A. van der Hucht, N. A. Miller +1 · 3 citations
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics and Star Formation Studies #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.1051/0004-6361:20077891
published as Astron.Astrophys.478:513,2008 · content: 11 pages, 4 figures
openalex publication_date 2007/12/04 · arxiv created 2008/03/06 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/04
We present XMM-Newton observations of the O supergiant ζ Orionis (O9.7 Ib). The spectra are rich in emission lines over a wide range of ionization stages. The rgs spectra show for the first time lines of low ion stages such as , , , and . The line profiles are symmetric and rather broad ( km s-1) and show only a slight blue shift. With the XMM-epic spectrometer several high ions are detected in this star for the first time including and . Simultaneous multi-temperature fits and DEM-modeling were applied to the rgs and epic spectra to obtain emission measures, elemental abundances and plasma temperatures. The calculations show temperatures in the range ≈0.07-0.6 keV. According to the derived models the intrinsic source X-ray luminosity at a distance of 251 pc is Lx = 1.37(.03) 1032 erg s-1 in the energy range 0.3-10 keV. In the best multi-temperature model fit, the abundances of C, N, O, and Fe are near their solar values, while the abundances of Ne, Mg, and Si appear somewhat enhanced. The sensitivity of the He-like forbidden and intercombination lines to ζ Ori's strong radiation field is used to derive the radial distances at which lines are formed. Values of 34 for , 12.5 for , 4.8 for , and 3.9 for are obtained.