Simulated X-ray emission for a runaway model of Kepler's supernova remnant

Fil:Velázquez, P.F. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina.

Guardado en:

Detalles Bibliográficos
Autores principales:	Velázquez, Pablo Fabián, Vigh, Carlos Donato, Reynoso, Estela Marta, Gomez, Daniel Osvaldo
Publicado:	2006
Materias:	Hydrodynamics ISM: individual (Kepler SNR) Methods: numerical Shock waves Supernova remnants X-rays: ISM
Acceso en línea:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v649_n2_p779_Velazquez http://hdl.handle.net/20.500.12110/paper_0004637X_v649_n2_p779_Velazquez
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

Ejemplares similares

Simulated X-ray emission for a runaway model of Kepler's supernova remnant
por: Velázquez, P.F., et al.
Publicado: (2006)

Simulated X-ray emission for a runaway model of Kepler's supernova remnant
por: Velázquez, P.F., et al.

Simulated X-ray emission for a runaway model of Kepler's supernova remnant
por: Velázquez, P.F., et al.
Publicado: (2006)

Study of the Rayleigh-Taylor instability in Tycho's supernova remnant
por: Velázquez, P.F., et al.

Study of the Rayleigh-Taylor instability in Tycho's supernova remnant
Publicado: (1998)

Asymmetries in the expansion and emission from young supernova remnants
por: Vigh, C.D., et al.

A new determination of the distance to Kepler's supernova remnant
por: Reynoso, E.M., et al.

A new determination of the distance to Kepler's supernova remnant
Publicado: (1999)

Asymmetries in the expansion and emission from young supernova remnants
Publicado: (2011)

A 3D numerical model for Kepler's supernova remnant
por: Velázquez, Pablo Fabián, et al.
Publicado: (2014)

A 3D numerical model for Kepler's supernova remnant
por: Toledo-Roy, J.C., et al.

Accounting for the foreground contribution to the dust emission towards Kepler's supernova remnant
por: Reynoso, Estela Marta
Publicado: (2009)

Accounting for the foreground contribution to the dust emission towards Kepler's supernova remnant
por: Gomez, H.L., et al.
Publicado: (2009)

Accounting for the foreground contribution to the dust emission towards Kepler's supernova remnant
por: Gomez, H.L., et al.

Accounting for the foreground contribution to the dust emission towards Kepler's supernova remnant
por: Gomez, H.L., et al.
Publicado: (2009)

Supernova remnants and the interstellar medium
Publicado: (1996)

Supernova remnants and the interstellar medium
por: Dubner, G.M.

Radio emission from supernova remnants
Publicado: (2015)

Radio emission from supernova remnants
por: Dubner, G., et al.

Effects of thermal conduction on the X-ray and synchrotron emission from supernova remnants
por: Velázquez, P.F., et al.

Neutral hydrogen in the direction of the Vela supernova remnant
Publicado: (1998)

Neutral hydrogen in the direction of the Vela supernova remnant
por: Dubner, G.M., et al.

Effects of thermal conduction on the X-ray and synchrotron emission from supernova remnants
Publicado: (2004)

Cosmic-ray acceleration at the forward shock in Tycho's supernova remnant: Evidence from Chandra X-ray observations
por: Warren, J.S., et al.

Cosmic-ray acceleration at the forward shock in Tycho's supernova remnant: Evidence from Chandra X-ray observations
Publicado: (2005)

CO observations toward supernova remnants with associated OH 1720 MHz masers
por: Reynoso, E.M., et al.

A blowout numerical model for the supernova remnant G352.7-0.1
por: Toledo-Roy, J.C., et al.

The molecular clouds in the environs of the supernova remnants G349.7+0.2 and G18.8+0.3
por: Dubner, G., et al.

A blowout numerical model for the supernova remnant G352.7-0.1
Publicado: (2013)

CO observations toward supernova remnants with associated OH 1720 MHz masers
Publicado: (2000)

An atomic and molecular study of the interstellar medium around the supernova remnant RCW 103
por: Paron, S.A., et al.

The supernova remnant W44: Confirmations and challenges for cosmic-ray acceleration
Publicado: (2014)

The supernova remnant W44: Confirmations and challenges for cosmic-ray acceleration
por: Cardillo, M., et al.

The molecular clouds in the environs of the supernova remnants G349.7+0.2 and G18.8+0.3
Publicado: (2004)

The environs of tycho's supernova remnant explored through the H I 21 centimeter line
por: Reynoso, E.M., et al.

The propagation of the shock wave from a strong explosion in a plane-parallel stratified medium: The Kompaneets approximation
por: Olano, Carlos Alberto
Publicado: (2009)

Indications of a Si-rich bilateral jet of ejecta in the Vela SNR observed with XMM-Newton
por: García, F, et al.
Publicado: (2017)

Isolated X-ray-infrared sources in the region of interaction of the supernova remnant IC 443 with a molecular cloud
Publicado: (2008)

Isolated X-ray-infrared sources in the region of interaction of the supernova remnant IC 443 with a molecular cloud
por: Bykov, A.M., et al.

Investigation of the large-scale neutral hydrogen near the supernova remnant W28
por: Velázquez, P.F., et al.