Published September 21, 2012
| Version v1
Technical note
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Nova Mon 2012 resolved as a double radio source
Authors/Creators
- 1. The University of Manchester
- 2. Joint Institute for VLBI in Europe (JIVE)
- 3. Michigan State/NRAO
- 4. NRC/NRL
- 5. Minnesota
- 6. NRAO
- 7. University of New Mexico
- 8. Columbia
- 9. UMBC/GSFC
- 10. Liverpool John Moores
- 11. Central Lancashire
Description
Nova Mon 2012 was first reported as a gamma-ray transient, subsequently associated with an optical nova and detected in the radio and X-ray/UV. Following the dramatic brightening at high radio frequencies, on September 18 we obtained e-VLBI radio observations of Nova Mon 2012 at 5.0 GHz using eight telescopes of the European VLBI Network (EVN), providing resolution of 6x8 milli-arcseconds.
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