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Cassiopeia A | | 800 km s-1 | | celestial sphere | | radio source catalog | | | | X-ray | | | X-ray source | 3U 2321+58 | A radio source in Cassiopeia, the strongest extrasolar source in the sky, believed to be the remnant of a Type II supernova whose light reached Earth about 1667. Optically it is a faint nebula. It has a mass of a few solar masses. It is also an extended source of soft X-rays. | 3 kpc | |
Centaurus A | | | | celestial sphere | | radio source catalog | | | | X-ray | | | X-ray source | NGC 5128 | A strong radio source. Optically, it is an elliptical galaxy with a dark obscuring lane. It is the nearest known violent galaxy. | 4 Mpc | |
Lupus Loop | | | | celestial sphere | | radio source catalog | | | | radio | | | radio source | | A radio source, a large broken shell 4°.5 in diameter, identified as a prehistoric supernova remnant. | | |
North Polar Spur | | | | celestial sphere | | radio source catalog | | | | X-ray | | | X-ray source | | A radio continuum feature extending from the galactic plane to the vicinity of the North Galactic Pole. It is believed to be a supernova remnant. It is also an X-ray source. | 50-200 pc | |
Orion A | | | | celestial sphere | | radio source catalog | | | | radio | | | radio source | | A radio continuum feature (an H II region) centered on the Trapezium, and excited by θ1 Ori C. The Orion A molecular cloud, which lies beyond it, is a rich source of molecules CO, OH, HCN, and probably NO, HCO, and H2CO have been observed. | | |
Orion B | | | | celestial sphere | | radio source catalog | | | | radio | | | radio source | NGC 2024 | A radio continuum source. | | |
radio galaxy | | | | celestial sphere | radio source | galaxy catalog | | 106 to 1012 | | radio | | | | | A galaxy that is extremely luminous at radio wavelengths. A radio galaxy is usually a giant elliptical - the largest galaxy in a cluster - and is a strong emitter of synchrotron radiation. M87 and M82 are examples. | | |
radio lobes | | | | celestial sphere | | radio source catalog | | | | radio | | | radio source | | Extended regions of diffuse radio emission, often dumbbell shaped, that surround a radio galaxy. | | |
Sagittarius A | | | | celestial sphere | | radio source catalog | | | | radio | | 12 pc | radio source | | The very center of the Milky Way, Sagittarius A* is a strong source of radio waves and probably a massive black hole. | | |
Sagittarius B2 | | | | celestial sphere | | radio source catalog | | | | radio | | | radio source | | A massive (3 × 106 Msun), dense (up to 108 particles per cm3) H II region and molecular cloud complex - the richest molecular source in the Galaxy. It is in the galactic plane, near the galactic center. | 10 kpc distant | |
supernova remnant | 10000 km s-1 | | | gas | radio source | radio source catalog | | | SNR | radio | 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 |
W3 | | | | celestial sphere | | radio source catalog | | | | radio | | | radio source | | A dense cloud of gas in the Perseus arm. | 3 kpc | |
W49 | | | | celestial sphere | | radio source catalog | | | | radio | | | radio source | | A radio source (a giant H II region). It is the most powerful thermal radio source known in our Galaxy. | 14 kpc | |