- Artículo:
A 300-parsec-long jet-inflated bubble around a powerful microquasar in the galaxy NGC 7793
- Autor:
Manfred W. Pakull
Roberto Soria
Christian Motch
- Resumen:
Ultraluminous X-ray sources are the most luminous class of black hole located outside the nuclei of active galaxies. They are often associated with shock-ionized nebulae, though with no evidence of collimated jets. Now, however, it is reported that the large nebula S26 in the nearby galaxy NGC 7793 is powered by a black hole with a pair of collimated jets. The jets seem to be 104 times more energetic than the X-ray emission from the core.
- Página:
209
- Publicación:
Nature
- Volúmen:
466
- Número:
7303
- Periodo:
8 Julio 2010
- ISSN:
00280836
- SrcID:
00280836-2010-07-08.txt
- Documento número 1206855
- Actualizado el martes, 10 de julio de 2018 11:34:00 a. m.
- Creado el martes, 10 de julio de 2018 11:34:00 a. m.
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