Far infrared observations of crab-like supernova remnants

Astronomy and Astrophysics – Astronomy

Scientific paper

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Crab Nebula, Infrared Astronomy, Pulsars, Radio Astronomy, Star Formation, Supernova Remnants, Synchrotron Radiation, Emission Spectra, H Ii Regions, Infrared Astronomy Satellite, Magnetic Fields, Thermal Emission, X Ray Spectra

Scientific paper

Using the Infrared Astronomy Satellite (IRAS) data, an investigation was begun of the far infrared properties of Crab-like supernova remnants and other synchrotron nebulae. Both the co-added scanning data and, where available, pointed observations were examined. To date infrared emission was found from two Crab-like remnants: G24.7+0.6 in which the infrared source near the center of the object was shown to be a compact HII region with EM greater than or approximately 10 to the 7th pc/cm(6); and G0.9+0.1 where a marginal detection of a 25 micron source coincident with the remnant core was used to set limits on the energetics of this synchrotron nebula. Further work, in progress under a second year of this program, should yield additional information concerning the distribution of initial pulsar spin periods and the evolution of synchrotron nebulae.

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