Hostname: page-component-745bb68f8f-5r2nc Total loading time: 0 Render date: 2025-01-10T01:52:46.077Z Has data issue: false hasContentIssue false
  • English
  • Français

Using stellar population studies to determine the progenitors of GRBs and SNe

Published online by Cambridge University Press:  13 April 2010

Christina C. Thöne ,
Lise Christensen  and
Johan P. U. Fynbo
Christina C. Thöne
Affiliation:
Istituto Nazionale di Astrofisica, Osservatorio Astronomico di Brera, Via E. Bianchi 46, 23807 Merate, Italy email: [email protected]
Lise Christensen
Affiliation:
European Southern Observatory, K. Schwarzschild Str. 1, 85748 Garching, Germany
Johan P. U. Fynbo
Affiliation:
Dark Cosmology Centre, Niels Bohr Institut, University of Copenhagen, Juliane Maries Vej 30, 2100 Copenhagen, Denmark
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present spatially resolved emission line studies of three nearby GRB and SN hosts with longslit and/or IFU observations. We compare the environment of the GRBs/SNe with those of other star-forming regions in the host galaxy and try to get informations on the progenitor from stellar population models and metallicities.

Keywords

galaxies:abundancesgamma-rays: burstsstars: supernovae: general
Type
Poster Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S262: Stellar Populations – Planning for the Next Decade , August 2009 , pp. 436 - 437
Copyright
Copyright © International Astronomical Union 2010

References

Galama, T. et al. 1998, Nature, 395, 670CrossRefGoogle Scholar
Fynbo, J. et al. 2006, Nature, 444, 1047CrossRefGoogle Scholar
Soderberg, A. et al. 2008, Nature, 454, 246CrossRefGoogle Scholar
Modjaz, M. et al. 2008, AJ, 135, 1136CrossRefGoogle Scholar
Christensen, L. et al. 2008, A&A, 490, 45Google Scholar
Thöne, et al. 2007, ApJ, 676, 1151CrossRefGoogle Scholar
Thöne, et al. 2009, ApJ, 698, 1207CrossRefGoogle Scholar