Supernovae play a prominent role in current theories of cosmology, galaxy evolution and stellar evolution. Key to understanding supernovae is a characterization of their progenitors. A robust body of theoretical work predicts the nature of these stars, but direct observations are lacking. Current theory and observations to date are summarized, as well as open questions in the field. Interferometric methods are proposed for the resolution of some of these questions
The recent discovery of the accelerating expansion of the Universe and thus the existence of dark en...
We present the results of our analysis of Hubble Space Telescope (HST) and deep ground-based images...
We present the results of our analysis of Hubble Space Telescope (HST) and deep ground-based images...
Supernovae (SNe) are the spectacular deaths of stars and have shaped the universe we see today. Thei...
Supernovae arise from progenitor stars occupying the upper end of the initial mass function. Their ...
Identifying the massive progenitor stars that give rise to core-collapse supernovae is one of the ma...
Supernovae are the explosive and luminous ends of life for a variety of types of star. They exhibit ...
Supernovae (SNe) are dramatic and violent end-points of stellar evolution, and lie at the heart of ...
A very active area of research in the field of core-collapse supernovae (SNe) is the study of their ...
Supernovae are intimately entwined with virtually all areas of astronomical research from the metal...
It is well-known that some massive stars evolve to an end state which results in the collapse of the...
Supernovae arise from progenitor stars occupying the upper end of the initial mass function. Their ...
A very active area of research in the field of core-collapse supernovae (SNe) is the study of their ...
A very active area of research in the field of core-collapse supernovae (SNe) is the study of their ...
Core-collapse supernovae (CCSNe) are an important part of the stellar evolution of massive stars. Ce...
The recent discovery of the accelerating expansion of the Universe and thus the existence of dark en...
We present the results of our analysis of Hubble Space Telescope (HST) and deep ground-based images...
We present the results of our analysis of Hubble Space Telescope (HST) and deep ground-based images...
Supernovae (SNe) are the spectacular deaths of stars and have shaped the universe we see today. Thei...
Supernovae arise from progenitor stars occupying the upper end of the initial mass function. Their ...
Identifying the massive progenitor stars that give rise to core-collapse supernovae is one of the ma...
Supernovae are the explosive and luminous ends of life for a variety of types of star. They exhibit ...
Supernovae (SNe) are dramatic and violent end-points of stellar evolution, and lie at the heart of ...
A very active area of research in the field of core-collapse supernovae (SNe) is the study of their ...
Supernovae are intimately entwined with virtually all areas of astronomical research from the metal...
It is well-known that some massive stars evolve to an end state which results in the collapse of the...
Supernovae arise from progenitor stars occupying the upper end of the initial mass function. Their ...
A very active area of research in the field of core-collapse supernovae (SNe) is the study of their ...
A very active area of research in the field of core-collapse supernovae (SNe) is the study of their ...
Core-collapse supernovae (CCSNe) are an important part of the stellar evolution of massive stars. Ce...
The recent discovery of the accelerating expansion of the Universe and thus the existence of dark en...
We present the results of our analysis of Hubble Space Telescope (HST) and deep ground-based images...
We present the results of our analysis of Hubble Space Telescope (HST) and deep ground-based images...