Modelling the circumstellar medium in RS Ophiuchi and its link to Type Ia supernovae
Recent interpretations of narrow, variable absorption lines detected in some Type Ia supernovae suggest that their progenitors are surrounded by dense, circumstellar material. Similar variations detected in the symbiotic recurrent nova system RS Oph, which undergoes thermonuclear outbursts every 20...
| Hoofdauteurs: | , , |
|---|---|
| Formaat: | Journal article |
| Gepubliceerd in: |
Oxford University Press
2016
|