A new young galactic supernova remnant containing a compact object: G15.9+0.2
We identify the radio-emitting shell-type supernova remnant G15.9+0.2 as a relatively young remnant containing an X-ray point source that may be its associated neutron star. The integrated spectrum of the remnant shell obtained from our 30 ks exploratory Chandra observation shows very strong lines t...
Guardado en:
| Autores principales: | Reynolds, S.P., Borkowski, K.J., Hwang, U.N.A., Harrus, I., Petre, R., Dubner, G. |
|---|---|
| Formato: | JOUR |
| Materias: | |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_0004637X_v652_n1II_pL45_Reynolds |
| Aporte de: |
Ejemplares similares
-
A new young galactic supernova remnant containing a compact object: G15.9+0.2
Publicado: (2006) -
Supernova Remnants Interacting with Molecular Clouds: X-Ray and Gamma-Ray Signatures
por: Slane, P., et al. -
Cosmic-ray acceleration at the forward shock in Tycho's supernova remnant: Evidence from Chandra X-ray observations
Publicado: (2005) -
Cosmic-ray acceleration at the forward shock in Tycho's supernova remnant: Evidence from Chandra X-ray observations
por: Warren, J.S., et al. -
Supernova Remnants Interacting with Molecular Clouds: X-Ray and Gamma-Ray Signatures
Publicado: (2015)