{ "id": "1507.05967", "version": "v1", "published": "2015-07-21T20:01:43.000Z", "updated": "2015-07-21T20:01:43.000Z", "title": "A spectroscopic survey of Herbig Ae/Be stars with X-Shooter I: Stellar parameters and accretion rates", "authors": [ "J. R. Fairlamb", "R. D. Oudmaijer", "I. Mendigutía", "J. D. Ilee", "M. E. van den Ancker" ], "comment": "29 pages, 19 figures, Accepted for publication in MNRAS", "categories": [ "astro-ph.SR" ], "abstract": "Herbig Ae/Be stars span a key mass range that links low and high mass stars, and thus provide an ideal window from which to explore their formation. This paper presents VLT/X-Shooter spectra of 91 Herbig Ae/Be stars, HAeBes; the largest spectroscopic study of HAeBe accretion to date. A homogeneous approach to determining stellar parameters is undertaken for the majority of the sample. Measurements of the ultra-violet (UV) are modelled within the context of magnetospheric accretion, allowing a direct determination of mass accretion rates. Multiple correlations are observed across the sample between accretion and stellar properties: the youngest and often most massive stars are the strongest accretors, and there is an almost 1:1 relationship between the accretion luminosity and stellar luminosity. Despite these overall trends of increased accretion rates in HAeBes when compared to classical T Tauri stars, we also find noticeable differences in correlations when considering the Herbig Ae and Herbig Be subsets. This, combined with the difficulty in applying a magnetospheric accretion model to some of the Herbig Be stars, could suggest that another form of accretion may be occurring within the Herbig Be mass range.", "revisions": [ { "version": "v1", "updated": "2015-07-21T20:01:43.000Z" } ], "analyses": { "keywords": [ "stellar parameters", "spectroscopic survey", "herbig ae/be stars span", "mass range", "high mass stars" ], "note": { "typesetting": "TeX", "pages": 29, "language": "en", "license": "arXiv", "status": "editable" } } }