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      • The new Chandra image provides new insight into the nature of SN 1006, which is the remnant of a so-called Type Ia supernova. This class of supernova is caused when a white dwarf pulls too much mass from a companion star and explodes, or when two white dwarfs merge and explode.
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  2. Apr 17, 2013 · The new Chandra image provides new insight into the nature of SN 1006, which is the remnant of a so-called Type Ia supernova. This class of supernova is caused when a white dwarf pulls too much mass from a companion star and explodes, or when two white dwarfs merge and explode.

  3. Sep 26, 2012 · Astronomers know that it was a type Ia supernova – a particular type of stellar sticky end that involves taking another star along for the ride.

  4. May 23, 2018 · To some modern investigators, this particular report represents probable evidence that the event was indeed a Type Ia supernova that was bright enough for its light to have cast shadows in the daytime- as is mentioned in several historical accounts.

  5. Aug 30, 2022 · Here, the authors show that SN 1006 remnant is an efficient source of cosmic rays, providing observational support for the quasi-parallel acceleration mechanism.

  6. Apr 18, 2013 · The Chandra image provides new insight into the nature of SN1006, which is the remnant of a so-called Type Ia supernova. This class of supernova is caused when a white dwarf pulls too much mass from a companion star and explodes, or when two white dwarfs merge and explode.

  7. Apr 18, 2013 · Chandra’s new image of the supernova remnant SN 1006 is the most spatially detailed map yet of the material ejected during a type Ia supernova.

  8. Nov 4, 2013 · SN 1006 (also known as SNR G.327.6+14.6) is the remnant of a Type Ia supernova that occurred some 7,200 light-years away from Earth in the southern constellation of Lupus (the Wolf). The supernova was widely seen on Earth in the year 1006 A.D. and is currently about 70 light-years across.

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