A blue point source at the location of supernova 2011DH
We present <i>Hubble Space Telescope</i> (HST) observations of the field of the Type IIb supernova (SN) 2011dh in M51 performed at ≈1161 rest-frame days after explosion using the Wide Field Camera 3 and near-UV filters F225W and F336W. A star-like object is detected in both bands and the...
Guardado en:
| Autores principales: | Folatelli, Gastón, Bersten, Melina Cecilia, Benvenuto, Omar Gustavo, Van Dyk, Schuyler D., Kuncarayakti, Hanindyo, Maeda, Keiichi, Nozawa, Takaya, Nomoto, Ken’ichi, Hamuy, Mario, Quimby, Robert M. |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2014
|
| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/84973 |
| Aporte de: |
Ejemplares similares
-
A binary progenitor for the type IIb supernova 2011dh in M51
por: Benvenuto, Omar Gustavo, et al.
Publicado: (2013) -
The type IIB supernova 2011DH from a supergiant progenitor
por: Bersten, Melina Cecilia, et al.
Publicado: (2012) -
A supergiant progenitor for SN 2011dh
por: Bersten, Melina Cecilia, et al.
Publicado: (2011) -
Late-time spectral line formation in Type IIb supernovae, with application to SN 1993J, SN 2008ax, and SN 2011dh
por: Jerkstrand, A., et al.
Publicado: (2015) -
The progenitor of the type IIb SN 2008ax revisited
por: Folatelli, Gastón, et al.
Publicado: (2015)