Suzaku studies supernova ‘crime scene,’ shows a single white dwarf to blame
MEXICO: “Mounting evidence indicates both of these mechanisms produce what we contact kind Ia supernovae,” mentioned lead researcher Hiroya Yamaguchi, an astrophysicist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “To realize how these stars explode, we need to study the debris in detail with sensitive instruments like these on Suzaku.”
The researchers analyzed archival observations of a supernova remnant named 3C 397, which is positioned about 33,000 light-years away in the constellation Aquila. Astronomers estimate this cloud of stellar debris has been expanding for amongst 1,000 and 2,000 years, creating 3C 397 a middle-aged remnant.
The team produced clear detections of components crucial to weighing the white dwarf utilizing information from Suzaku’s X-ray Imaging Spectrometer. The observation, created in October 2010 at energies in between 5,000 and 9,000 electron volts, provided a total productive exposure of 19 hours.
Infrared information from NASA’s Spitzer Space Telescope provided insight into the amount of gas and dust the expanding remnant has gathered up as it drives into interstellar space. The observations, from April 2005, indicate 3C 397 has swept up a mass some 18 instances greater than the original white dwarf. As a outcome, the group concludes that shock waves have thoroughly heated the remnant’s innermost parts.
Most low- and medium-mass stars related to the sun will end their days as white dwarfs. A common white dwarf is about as massive as our sun however roughly the size of Earth. This tends to make white dwarfs among the densest objects scientists know of, surpassed only by neutron stars and black holes.
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