Infinite photos and videos for every Wiki article · Find something interesting to watch in seconds
Infinite photos and videos for every Wiki article · Find something interesting to watch in seconds
The blue and green are optical images of the field in which the black widow pulsar is found, the green indicating the H-alpha bow shock. The red and w
The blue and green are optical images of the field in which the black widow pulsar is found, the green indicating the H-alpha bow shock. The red and white are the colors of the shock structures discovered in x-ray by the Chandra X-ray Observatory.
Artist's impression of the pulsar surrounded by its bow shock. White rays indicate particles of matter and antimatter being spewed from the star. Its
Artist's impression of the pulsar surrounded by its bow shock. White rays indicate particles of matter and antimatter being spewed from the star. Its companion star is too close to the pulsar to be visible at this scale.
Depiction of the same pulsar one million times closer showing the effect of its wind on its companion star, which is evaporating. The bow shock is too
Depiction of the same pulsar one million times closer showing the effect of its wind on its companion star, which is evaporating. The bow shock is too large to be shown, and at this scale would extend more than 15 miles (24 km) beyond the edge of the computer screen.
Sagitta
Sagitta can be seen above Aquila in this plate from Urania's Mirror (1825).
Messier 71 globular cluster
Messier 71 globular cluster
James Webb Space Telescope image of WR 124 in Sagitta. NIRCam and MIRI composite
James Webb Space Telescope image of WR 124 in Sagitta. NIRCam and MIRI composite