{ "id": "1304.5965", "version": "v1", "published": "2013-04-22T14:38:16.000Z", "updated": "2013-04-22T14:38:16.000Z", "title": "Footprints in the wind of Vela X-1 traced with MAXI", "authors": [ "V. Doroshenko", "A. Santangelo", "S. Nakahira", "T. Mihara", "M. Sugizaki", "M. Matsuoka", "M. Nakajima", "K. Makishima" ], "comment": "5 pages, 3 figures, accepted in A&A", "categories": [ "astro-ph.HE" ], "abstract": "The stellar wind around the compact object in luminous wind-accreting high mass X-ray binaries is expected to be strongly ionized with the X-rays coming from the compact object. The stellar wind of hot stars is mostly driven by light absorption in lines of heavier elements, and X-ray photo-ionization significantly reduces the radiative force within the so-called Stroemgren region leading to wind stagnation around the compact object. In close binaries like Vela X-1 this effect might alter the wind structure throughout the system. Using the spectral data from Monitor of All-sky X-ray Image (MAXI), we study the observed dependence of the photoelectric absorption as function of orbital phase in Vela X-1, and find that it is inconsistent with expectations for a spherically-symmetric smooth wind. Taking into account previous investigations we develop a simple model for wind structure with a stream-like photoionization wake region of slower and denser wind trailing the neutron star responsible for the observed absorption curve.", "revisions": [ { "version": "v1", "updated": "2013-04-22T14:38:16.000Z" } ], "analyses": { "keywords": [ "compact object", "wind-accreting high mass x-ray binaries", "wind structure", "stellar wind", "footprints" ], "tags": [ "journal article" ], "publication": { "doi": "10.1051/0004-6361/201321305", "journal": "Astronomy and Astrophysics", "year": 2013, "month": "Jun", "volume": 554 }, "note": { "typesetting": "TeX", "pages": 5, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1229295, "adsabs": "2013A&A...554A..37D" } } }