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XMM-Newton's Views of SN 1979C in M100: The supernova that just won't fade away

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Minimum credit line: Image courtesy of Stefan Immler (NASA GSFC) and ESA. (for details, see Conditions of Use).
Credit: ESA/XMM-Newton, CC BY-SA 3.0 IGO

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About this Image

These false-colour images show the spiral galaxy M100, also known as NGC 4321, and within the galaxy the supernova SN 1979C. On the left is the image of M100 in the UV/optical, taken with XMM-Newton's Optical Monitor (OM) camera, and on the right the galaxy is shown on the same scale but imaged in the X-ray with XMM-Newton's MOS cameras. M100 is in the Virgo cluster of galaxies, 56 million light years from Earth. The overall appearance of the galaxy is strikingly different in the X-ray compared to the UV/optical. The OM image clearly shows the spiral structure of the galaxy whilst in the X-ray image this structure is not visible and instead the galaxy X-ray luminosity tends to fall off from the galaxy centre, with some bright regions. The supernova 1979C is shown circled in the UV/optical image, and can be seen as an orange spot to the lower left of the galactic centre (which appears white) in the X-ray image. This particular supernova is curious because it is still just as bright in the X-ray as when it was observed by ROSAT in 1995, six years before the XMM-Newton observation. Normally objects of this type would be expected to dim significantly over time. In the OM image the false colouring was done using images taken with three fiters: the B filter (4340 Å), the U filter (3440 Å) and the UVW1 (2910 Å). In the X-ray image soft (0.3-1.5 keV) X-rays are shown in red, medium (1.5-4 keV) in green and hard (4-10 keV) in blue. The hardest X-rays are emitted from the galactic core, but are not seen as pure blue because there are also medium and soft X-rays emitted from that location.

Investigator(s):  S. Immler, R. A. Fesen, S. D. Van Dyk, K. W. Weiler, R. Petre, W. H. G. Lewin, D. Pooley, W. Pietsch, B. Aschenbach, M. C. Hammell, G. C. Rudie

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