chandra_614 December 10th, 2015
Credit: Wide Field Optical: Focal Pointe Observatory/B.Franke, Inset: X-ray: NASA/CXC /MSFC/D.Swartz et al, Inset: Optical: DSS, SARA
The Jellyfish Nebula is the remnant of a supernova that occurred over 10,000 years ago in our galaxy. New Chandra observations show that a peculiar object located on the southern edge of the remnant is likely a pulsar and may have formed in the explosion that created the Jellyfish Nebula. This new composite image shows the spectacular filamentary structure of IC 443 in a wide-field view from an amateur astrophotographer. Within the inset box, another optical image from the Digitized Sky Survey (red, green, orange, and cyan) has been combined with X-ray data from Chandra (blue). The inset shows a close-up view of the region around the pulsar candidate.
Provider: Chandra X-ray Observatory
Image Source: http://chandra.harvard.edu/photo/2015/ic443/
Curator: Chandra X-ray Observatory, Cambridge, MA, USA
Image Use Policy: http://chandra.harvard.edu/photo/image_use.html
Telescope | Spectral Band | Wavelength | |
---|---|---|---|
Focal Pointe Observatory (Takahashi FSQ-106ED) | Optical (SII) | 673.0 nm | |
Focal Pointe Observatory (Takahashi FSQ-106ED) | Optical (Ha) | 656.0 nm | |
Focal Pointe Observatory (Takahashi FSQ-106ED) | Optical (OIII) | 437.0 nm | |
Chandra (ACIS) | X-ray (X-ray) | 826.7 pm | |
DSS (DSS2R) | Optical (R-band) | 660.0 nm | |
DSS (DSS2IR) | Optical (IR-band) | 798.0 nm | |
SARA (0.9m Kitt Peak) | Optical (H-alpha) | 656.0 nm | |
SARA (0.9m Kitt Peak) | Optical (OIII) | 437.0 nm | |
First three entries in each field describe the wide field image. |
Detailed color mapping information coming soon...
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