Astronomers have captured supernova remnant, called G299.2-2.9, which looked like a blooming comic flower from Earth.
Image Credit: NASA/CXC/U.Texas
Astronomers have captured supernova remnant, called G299.2-2.9, which looked like a blooming comic flower from Earth.
Because the debris fields of exploded stars, known as supernova remnants, are very hot, energetic, and glow brightly in X-ray light, NASA's Chandra X-ray Observatory has proven to be a valuable tool in studying them. The supernova remnant called G299.2-2.9 (or G299 for short) is located within Earth's Milky Way galaxy, but Chandra's new image of it is reminiscent of a beautiful flower here on Earth.
G299 was left over by a particular class of supernovas called Type Ia. Astronomers think that a Type Ia supernova is a thermonuclear explosion, involving the fusion of elements and release of vast amounts of energy, of a white dwarf star in a tight orbit with a companion star.
If the white dwarf's partner is a typical, Sun-like star, the white dwarf can become unstable and explode as it draws material from its companion. Alternatively, the white dwarf was in orbit with another white dwarf, the two may merge and can trigger an explosion.
In this new Chandra image, red, green, and blue represent low, medium, and high-energy X-rays, respectively, detected by the telescope. The medium energy X-rays include emission from iron, and the hard-energy X-rays include emission from silicon and sulfur. The X-ray data have been combined with infrared data from the ground-based 2MASS survey that shows the stars in the field of view.
By performing a detailed analysis of the X-rays, researchers found several clear examples of asymmetry in G299. For example, the ratio between the amounts of iron and silicon in the part of the remnant just above the center is larger than in the part of the remnant just below the center.
This difference can be seen in the greener color of the upper region compared to the bluer color of the lower region. Also, there is a strongly elongated portion of the remnant extending to the right. In this region, the relative amount of iron to silicon is similar to that found in the southern region of the remnant.
The patterns seen in the Chandra data suggest that a very lopsided explosion may have produced this Type Ia supernova. It might also be that the remnant has been expanding into an environment where the medium it encountered was uneven. Regardless of the ultimate explanation, observations of G299 and others like it are showing astronomers just how varied such beautiful cosmic flowers can be.
via Science - Google News http://ift.tt/1yzXwWZ
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