Journal article
VLBI observations of SN 2008iz: I. Expansion velocity and limits on anisotropic expansion
Astronomy and astrophysics (Berlin), Vol.516(18), p.A27
03/24/2010
DOI: 10.1051/0004-6361/201014133
Abstract
We present observations of the recently discovered supernova 2008iz in M82
with the VLBI High Sensitivity Array at 22 GHz, the Very Large Array at
frequencies of 1.4, 4.8, 8.4, 22 and 43 GHz, and the Chandra X-ray observatory.
The supernova was clearly detected on two VLBI images, separated by 11 months.
The source shows a ring-like morphology and expands with a velocity of ~23000
km/s. The most likely explosion date is in mid February 2008. The measured
expansion speed is a factor of ~2 higher than expected under the assumption
that synchrotron self-absorption dominates the light curve at the peak,
indicating that this absorption mechanism may not be important for the radio
emission. We find no evidence for an asymmetric explosion. The VLA spectrum
shows a broken power law, indicating that the source was still optically thick
at 1.4 GHz in April 2009. Finally, we report upper limits on the X-ray emission
from SN 2008iz and a second radio transient recently discovered by MERLIN
observations.
Details
- Title: Subtitle
- VLBI observations of SN 2008iz: I. Expansion velocity and limits on anisotropic expansion
- Creators
- A Brunthaler - Max Planck SocietyI Marti-Vidal - Max Planck Institute for Radio AstronomyK. M Menten - Max Planck SocietyM. J Reid - Harvard UniversityC Henkel - Max Planck SocietyG. C Bower - University of California, BerkeleyH Falcke - ASTRONH Feng - Tsinghua UniversityP Kaaret - University of IowaN. R Butler - University of California, BerkeleyA. N Morgan - University of California, BerkeleyA Weiss - Max Planck Society
- Resource Type
- Journal article
- Publication Details
- Astronomy and astrophysics (Berlin), Vol.516(18), p.A27
- DOI
- 10.1051/0004-6361/201014133
- ISSN
- 0004-6361
- eISSN
- 1432-0746
- Language
- English
- Date published
- 03/24/2010
- Academic Unit
- Physics and Astronomy
- Record Identifier
- 9984199791402771
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