Copy reference, caption or embed code

Figure 3 - A Broadband X-Ray Study of the Rabbit Pulsar Wind Nebula Powered by PSR J1418-6058

Figure 3. An observed "on−off" image (left) and a simulated image of J1418 +X1 (right). Left: An exposure-scaled off-pulse image is subtracted from an on-pulse one in the 10-30 keV band. Right: A simulated image of the pulsar (center) and X1 (west) assuming that X1 was as bright as was seen in the XMM-Newton data. X1 is placed at ∼21″ northwest of J1418 (as observed by XMM-Newton). R = 30″ white circles are shown for reference, the figures are smoothed, and scales are adjusted for better legibility.
An observed "on−off" image (left) and a simulated image of J1418 +X1 (right). Left: An exposure-scaled off-pulse image is subtracted from an on-pulse one in the 10-30 keV band. Right: A simulated image of the pulsar (center) and X1 (west) assuming that X1 was as bright as was seen in the XMM-Newton data. X1 is placed at ∼21″ northwest of J1418 (as observed by XMM-Newton). R = 30″ white circles are shown for reference, the figures are smoothed, and scales are adjusted for better legibility.
Go to figure page
Reference
Caption
Embed code