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physical object > natural object > celestial body > nebula > H II region > gaseous nebula > expanding emission nebula > supernova remnant > Cygnus Loop
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Cygnus Loop comparison table
Subject has ejection velocity is part of is a kind of has catalog has wavelength has acronym produce is an instance of has synonym has image has definition has distance has age has composition
supernova remnant10000 km s-1gasradio sourceradio source catalogradioSNRsynchrotron radiation emission nebula A gaseous nebula, the expanding shell ejected by a supernova, and deriving its energy (at least in some cases) from the conversion by the remanent neutron star of its rotational energy into a stream of high-energy particles being continually accelerated in the SNR. About 100 SNRs are known in our Galaxy. Supernova remnants are usually powerful radio sources.  enhanced with heavy elements relative to the interstellar medium
X-ray source celestial spherecelestial body X-ray     A class of celestial objects whose dominant mechanism of energy dissipation is through X-ray emission. Galactic X-ray sources appear optically as starlike objects, peculiar in their ultraviolet intensity, variability (on time scales ranging from milliseconds to weeks), and spectral features. All known compact X-ray sources are members of close binary systems; a current popular model is mass accretion onto a compact object from a massive companion. (Four X-ray sources - all variable - are known to be associated with globular clusters.) The 21 known extended X-ray sources associated with clusters of galaxies seem to be clouds of hot gas trapped in the cluster's gravitational field.   
Cygnus Loop10000 km s-1gas radio source catalogX-raySNRsynchrotron radiationX-ray sourceCygnus X-5A supernova remnant, consisting of a large loop of gas ejected from a star. It is 100 pc above the galactic plane. (X-ray observations give a distance of 2-3 kpc.) It is a thermal bremsstrahlung source of soft X-rays with a spectral temperature of 2 × 106 K.770 pc20000 yearsenhanced with heavy elements relative to the interstellar medium

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