{ "id": "1606.02285", "version": "v1", "published": "2016-06-07T19:59:59.000Z", "updated": "2016-06-07T19:59:59.000Z", "title": "On the detectability of CO molecules in the Interstellar Medium via X-ray spectroscopy", "authors": [ "Katerine Joachimi", "Efraín Gatuzz", "Javier A. García", "Timothy R. Kallman" ], "comment": "7 pages, 5 figures", "categories": [ "astro-ph.HE" ], "abstract": "We present a study of the detectability of CO molecules in the Galactic interstellar medium using high-resolution X-ray spectra obtained with the XMM-Newton Reflection Grating Spectrometer. We analyzed 10 bright low mass X-ray binaries (LMXBs) to study the CO contribution in their line-of-sights. A total of 25 observations were fitted with the ISMabs X-ray absorption model which includes photoabsorption cross-sections for O I, O II, O III and CO. We performed a Monte-Carlo (MC) simulation analysis of the goodness of fit in order to estimate the significance of the CO detection. We determine that the statistical analysis prevents a significant detection of CO molecular X-ray absorption features, except for the lines-of-sight toward XTE~J1718-330 and 4U~1636-53. In the case of XTE~J1817-330, this is the first report of the presence of CO along its line-of-sight. Our results reinforce the conclusion that molecules have a minor contribution to the absorption features in the O K-edge spectral region. We estimate a CO column density lower limit to perform a significant detection with XMM-Newton of N(CO) > 6x10^{16} cm-2 for typical exposure times", "revisions": [ { "version": "v1", "updated": "2016-06-07T19:59:59.000Z" } ], "analyses": { "keywords": [ "interstellar medium", "x-ray spectroscopy", "detectability", "bright low mass x-ray binaries", "molecular x-ray absorption features" ], "note": { "typesetting": "TeX", "pages": 7, "language": "en", "license": "arXiv", "status": "editable" } } }