{ "id": "1409.2684", "version": "v1", "published": "2014-09-09T11:16:18.000Z", "updated": "2014-09-09T11:16:18.000Z", "title": "A multi-wavelength view on the dusty Wolf-Rayet star WR 48a", "authors": [ "Svetozar A. Zhekov", "Toma Tomov", "Marcin P. Gawronski", "Leonid N. Georgiev", "Jura Borissova", "Radostin Kurtev", "Marc Gagne", "Marcin Hajduk" ], "comment": "Accepted for publication in MNRAS; 16 pages, 16 figures, 6 tables", "categories": [ "astro-ph.SR" ], "abstract": "We present results from the first attempts to derive various physical characteristics of the dusty Wolf-Rayet star WR 48a based on a multi-wavelength view of its observational properties. This is done on the basis of new optical and near-infrared spectral observations and on data from various archives in the optical, radio and X-rays. The optical spectrum of WR 48a is acceptably well represented by a sum of two spectra: of a WR star of the WC8 type and of a WR star of the WN8h type. The strength of the interstellar absorption features in the optical spectra of WR 48a and the near-by stars D2-3 and D2-7 (both members of the open cluster Danks 2) indicates that WR 48a is located at a distance of ~4 kpc from us. WR 48a is very likely a thermal radio source and for such a case and smooth (no clumps) wind its radio emission suggests a relatively high mass-loss rate of this dusty WR star (dM/dt = a few x 10^(-4) solar masses per year). Long timescale (years) variability of WR 48a is established in the optical, radio and X-rays. Colliding stellar winds likely play a very important role in the physics of this object. However, some LBV-like (luminous blue variable) activity could not be excluded as well.", "revisions": [ { "version": "v1", "updated": "2014-09-09T11:16:18.000Z" } ], "analyses": { "keywords": [ "dusty wolf-rayet star wr 48a", "multi-wavelength view", "wr star", "optical spectrum", "interstellar absorption features" ], "tags": [ "journal article" ], "publication": { "doi": "10.1093/mnras/stu1880", "journal": "Monthly Notices of the Royal Astronomical Society", "year": 2014, "month": "Dec", "volume": 445, "number": 2, "pages": 1663 }, "note": { "typesetting": "TeX", "pages": 16, "language": "en", "license": "arXiv", "status": "editable", "adsabs": "2014MNRAS.445.1663Z" } } }