We propose an in-depth X-ray study of fast-evolving, blue optical transients (FBOTs). FBOTs are a new class of explosions with luminosities and time scales of evolution that challenge traditional Supernova (SN) models. To date, FBOTs have mostly been studied in the optical/UV, which is of thermal origin and it is not sensitive to the nature of the underlying energy source and properties of the explosion’s fastest ejecta. Here we propose to capitalize on our recent Chandra discovery of the first X-ray emission from a FBOT and start the first X-ray monitoring campaign of nearby FBOTs. The primary goals are to (i) obtain the first constraints on the mass-loss history of the stellar progenitors of a new class of SN explosions; (ii) test the presence of engines driving the explosions.
|Effective start/end date||10/31/19 → 10/30/20|
- Smithsonian Astrophysical Observatory (G09-20054A//NAS8-03060)
- National Aeronautics and Space Administration (G09-20054A//NAS8-03060)