| | 21 | |
| | 22 | Type Ia Supernovae and Their Environments: Multi-Wavelength Constraints on |
| | 23 | Progenitor Systems |
| | 24 | |
| | 25 | |
| | 26 | |
| | 27 | |
| | 28 | To approach the Chandasekhar mass and explode as a Type Ia supernova, a white |
| | 29 | dwarf must accrete material from a binary companion. In most cases, this |
| | 30 | transfer of material should leave an imprint on the environment in the form of |
| | 31 | detectable circumbinary material. I will discuss multi-wavelength constraints on |
| | 32 | the environments of SNe Ia and the implications for progenitor systems, with |
| | 33 | particular focus on our deep radio observations with the JVLA. |