Volume 491, Number 1, November III 2008Diagnostics of interstellar hydrogen in the heliosphere
|Page(s)||189 - 207|
|Published online||23 September 2008|
High-ion absorption in seven GRB host galaxies at z = 2–4*
Evidence for both circumburst plasma and outflowing interstellar gas
European Southern Observatory, Alonso de Córdova 3107, Casilla 19001, Vitacura, Santiago, Chile e-mail: firstname.lastname@example.org
2 Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, 2100 Copenhagen, Denmark
3 Institute of Theoretical Astrophysics, University of Oslo, PO Box 1029, Blindern, 0315 Oslo, Norway
Accepted: 29 May 2008
Aims. We use VLT/UVES high-resolution optical spectroscopy of seven GRB afterglows (at zGRB between 2.20 and 3.97) to investigate circumburst and interstellar plasma in the host galaxies of the bursts.
Methods. GRBs 050730, 050820, 050922C, 060607, 071031, and 080310 were each detected by the Swift satellite. With the minimum possible time delay (as short as eight minutes), follow-up optical spectroscopy at 6.0 km s-1 resolution began with UVES. We present Voigt-profile component fits and analysis of the high-ion absorption detected in these spectra and in the pre-Swift UVES spectrum of GRB 021004, at velocities between zGRB–5000 km s-1 and zGRB.
Results. We identify several distinct categories of high-ion absorption at velocities close to zGRB: (i) strong high-ion absorption at zGRB itself is always seen in O vi, C iv, and Si iv, usually (in six of seven cases) in N v, and occasionally in S iv and S vi. Three of the cases show log N(N v) > 14 in a single-component, suggesting a circumburst origin, but we cannot rule out an interstellar origin. Indeed, using the non-detection of S iv* at zGRB toward GRB 050730 together with a UV photo-excitation model, we place a lower limit of 400 pc on the distance of the S iv-bearing gas from the GRB; (ii) complex, multi-component C iv and Si iv profiles extending over 100–400 km s-1 around zGRB are observed in each spectrum; these velocity fields are similar to those measured in C iv in damped Lyman-α systems at similar redshifts, suggesting a galactic origin; (iii) asymmetric, blueshifted, absorption-line wings covering 65–140 km s-1 are seen in the C iv, Si iv, and O vi profiles in four of the seven GRB afterglow spectra. The wing kinematics together with the “Galactic” C iv/Si iv ratios measured in two cases suggest that the wings trace outflowing interstellar gas in the GRB host galaxies; (iv) high-velocity (HV; 500–5000 km s-1 relative to zGRB) components are detected in six of the seven spectra; these components are not necessarily a single homogeneous population, and many of them may arise in unrelated foreground galaxies. However, in the cases of GRBs 071031 and 080310, the ionization properties of the HV components (very high C iv/Si iv ratios and absence of neutral-phase absorption in Si ii or C ii) are suggestive of a circumburst origin; models of Wolf-Rayet winds from the GRB progenitors can explain both the kinematics and ionization level of these HV components.
Key words: gamma rays: bursts / galaxies: halos / galaxies: high-redshift / galaxies: ISM / stars: Wolf-Rayet
© ESO, 2008
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.