Asimetric Supernova SN IA
Supernova asimetrica descubierta recientemente.
Las SN Ia deben ser fuertemente asimetricas, esto fue calculado usando un modelo de
deflagracion fractal. Hasta ahora las asimetrias detectadas en SN Ia eran pequeñas y podian ser explicadas por diversos modelos. Nuestros calculos muestran que esta asimetria puede ser mucho mayor, como la detectada recientemente en la
SNR 0104 Ver:
2004MNRAS.348..451G,
Ghezzi, C. R.; de Gouveia Dal Pino, E. M.; Horvath, J. E., "Asymmetric explosions of thermonuclear supernovae",
2001ApJ...548L.193G,
Ghezzi, Cristian R.; de Gouveia Dal Pino, Elisabete M.; Horvath, Jorge E., "Magnetic Field Effects on the Thermonuclear Combustion Front of Chandrasekhar Mass White Dwarfs"
A continuacion la noticia del descubrimiento astronomico:
A new image from NASA's Chandra X-ray Observatory shows a supernova remnant with a different look। This object, known as SNR 0104-72।3 (SNR 0104 for short), is in the Small Magellanic Cloud, a small neighboring galaxy to the Milky Way. Astronomers think that SNR 0104 is the remains of a so-called Type Ia supernova caused by the thermonuclear explosion of a white dwarf.
In this composite made of X-rays from Chandra shown in purple and infrared data from Spitzer shown in green and red, SNR 0104 looks unlike other likely Type Ia remnants found in our own Galaxy. While objects such as the Kepler and Tycho supernova remnants appear circular, the shape of SNR 0104 in X-rays is not.
Instead, the image is dominated by two bright lobes of emission (seen to the upper right and lower left). The large amount of iron in these lobes indicates that SNR 0104 was likely formed by a Type Ia supernova.
One possible explanation for this structure is that the explosion of the white dwarf itself was strongly asymmetrical and produced two jets of iron. Another possibility is that the complicated environment seen in the image is responsible. The green shells on the left and right side of SNR 0104 correspond to surrounding material that has been swept up by the explosion. So, the unusual shape of the remnant might be caused by a lack of material to the north and south of the star to interrupt the outward path of the stellar debris. This explanation, however, is still in question and scientists hope more data from Chandra and other telescopes will help settle the debate.
The presence of a nearby massive star and the shells of gas and dust seen in the wide-field view from Spitzer shows that SNR 0104 might be located within a star-forming region. This suggests that SNR 0104 may belong to a little-studied class of so-called "prompt"
Type Ia supernovas caused by the demise of younger, more massive stars than average. Again, more data will be needed to test this theory.
This research was led by Sangwook Park and Jae-Joon Lee of Penn State University and was presented at the 214th meeting of the American Astronomical Society in Pasadena, California. NASA's Marshall Space Flight Center in Huntsville, Ala., manages the Chandra program for NASA's Science Mission Directorate in Washington. The
Smithsonian Astrophysical Observatory controls Chandra's science and flight operations from Cambridge, Mass.
Title:
