Discovery of an extended X-ray jet in AP librae
dc.contributor.author | Kaufmann, S. | |
dc.contributor.author | Wagner, S. | |
dc.contributor.author | Tibolla, Omar | |
dc.date.accessioned | 2017-01-30T14:47:25Z | |
dc.date.available | 2017-01-30T14:47:25Z | |
dc.date.created | 2014-10-08T01:14:50Z | |
dc.date.issued | 2013 | |
dc.identifier.citation | Kaufmann, S. and Wagner, S. and Tibolla, O. 2013. Discovery of an extended X-ray jet in AP librae. Astrophysical Journal. 776 (2): pp. 1-7. | |
dc.identifier.uri | http://hdl.handle.net/20.500.11937/40988 | |
dc.description.abstract |
Chandra observations of the low-energy-peaked BL Lac object (LBL) AP Librae (AP Lib) revealed the clear discovery of a non-thermal X-ray jet. AP Lib is the first LBL with an extended non-thermal X-ray jet that shows emission into the very high energy range. The X-ray jet has an extension of ~15''(˜ 14 kpc). The X-ray jet morphology is similar to the radio jet observed with Very Large Array at 1.36 GHz emerging in the southeast direction and bends by 50° at a distance of 12'' toward the northeast. The intensity profiles of the X-ray emission studied are consistent with those found in the radio range. The spectral analysis reveals that the X-ray spectra of the core and jet region are both inverse-Compton-(IC)-dominated. This adds to a still small sample of BL Lac objects whose X-ray jets are IC-dominated and thus more similar to the high-luminosity Fanaroff-Riley II sources than to the low-luminosity Fanaroff-Riley I objects, which are usually considered to be the parent population of BL Lac objects. | |
dc.publisher | Institute of Physics Publishing, Inc. | |
dc.relation.uri | http://iopscience.iop.org/0004-637X/776/2/68/ | |
dc.title | Discovery of an extended X-ray jet in AP librae | |
dc.type | Journal Article | |
dcterms.source.volume | 776 | |
dcterms.source.number | 2 | |
dcterms.source.startPage | 1 | |
dcterms.source.endPage | 7 | |
dcterms.source.issn | 0004-637X | |
dcterms.source.title | Astrophysical Journal | |
curtin.accessStatus | Fulltext not available |