W49B

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Emission nebula
W49B

Supernova Remnant W49B in x-ray, radio, and infrared.jpg

Fog W49B
AladinLite
Constellation Eagle
Position
equinoxJ2000.0 , epoch : J2000.0
Right ascension 19 h 11 m 09 s
declination + 09 ° 06 ′ 24 ″
Appearance
Ionizing source
Physical data

distance  26000 ly
(8000 pc )
history
Catalog names

W49B (also SNR G043.3-00.2 or 3C 398 ) is a supernova remnant that arose from a Type Ib or Type Ic supernova. If this supernova could have been observed on Earth , around 1000 AD. Possibly a gamma-ray flash and a black hole arose from the supernova .

W49B is barrel-shaped and is approximately 8,000  parsecs (26,000 light years ) from Earth. In the infrared, ring-shaped structures are visible that surround the "barrel" and have a diameter of about 25 light years. In addition, forbidden lines of highly ionized nickel and iron were found in the X-ray area .

Individual evidence

  1. "The Galactic Supernova Remnant W49B Likely Originates from a Jet-driven, Core-collapse Explosion" by Laura A. Lopez ( Astrophysical Journal , 2013) doi : 10.1088 / 0004-637X / 764/1/50
  2. W49B: Did An Explosion Create Our Galaxy's Youngest Black Hole? February 13, 2013
  3. ^ "Baby black hole is swaddled in a supernova remnant" by Flora Graham, New Scientist , 2013