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physical object > natural object > celestial body > nebula > H II region > gaseous nebula > expanding emission nebula > supernova remnant > Cygnus Loop |
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 |
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supernova remnant | 10000 km s-1 | gas | radio source | radio source catalog | radio | SNR | synchrotron 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 sphere | celestial 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 Loop | 10000 km s-1 | gas | radio source catalog | X-ray | SNR | synchrotron radiation | X-ray source | Cygnus X-5 | A 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 pc | 20000 years | enhanced with heavy elements relative to the interstellar medium |
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