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A massive runaway star from 30 doradus

Evans, CJ, Walborn, NR, Crowther, PA, Hénault-Brunet, V, Massa, D, Taylor, WD, Howarth, ID, Sana, H, Lennon, DJ and Van Loon, JT (2010) A massive runaway star from 30 doradus Astrophysical Journal Letters, 715 (2 PART).

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Abstract

We present the first ultraviolet (UV) and multi-epoch optical spectroscopy of 30 Dor 016, a massive O2-type star on the periphery of 30 Doradus in the Large Magellanic Cloud. The UV data were obtained with the Cosmic Origins Spectrograph on the Hubble Space Telescope as part of the Servicing Mission Observatory Verification program after Servicing Mission 4, and reveal #016 to have one of the fastest stellar winds known. From analysis of the C IV λλ1548-51 doublet we find a terminal velocity, v ∞ = 3450 50km s-1. Optical spectroscopy is from the VLT-FLAMES Tarantula Survey, from which we rule out a massive companion (with 2days<P<1yr) to a confidence of 98%. The radial velocity of #016 is offset from the systemic value by -85km s-1, suggesting that the star has traveled the 120pc from the core of 30 Doradus as a runaway, ejected via dynamical interactions. © 2010 The American Astronomical Society. All rights reserved.

Item Type: Article
Authors :
NameEmailORCID
Evans, CJUNSPECIFIEDUNSPECIFIED
Walborn, NRUNSPECIFIEDUNSPECIFIED
Crowther, PAUNSPECIFIEDUNSPECIFIED
Hénault-Brunet, VUNSPECIFIEDUNSPECIFIED
Massa, DUNSPECIFIEDUNSPECIFIED
Taylor, WDUNSPECIFIEDUNSPECIFIED
Howarth, IDUNSPECIFIEDUNSPECIFIED
Sana, HUNSPECIFIEDUNSPECIFIED
Lennon, DJUNSPECIFIEDUNSPECIFIED
Van Loon, JTUNSPECIFIEDUNSPECIFIED
Date : 1 January 2010
Identification Number : https://doi.org/10.1088/2041-8205/715/2/L74
Depositing User : Symplectic Elements
Date Deposited : 17 May 2017 12:54
Last Modified : 17 May 2017 12:54
URI: http://epubs.surrey.ac.uk/id/eprint/837184

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