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dc.contributor.authorKaufmann, S.
dc.contributor.authorWagner, S.
dc.contributor.authorTibolla, Omar
dc.date.accessioned2017-01-30T14:47:25Z
dc.date.available2017-01-30T14:47:25Z
dc.date.created2014-10-08T01:14:50Z
dc.date.issued2013
dc.identifier.citationKaufmann, 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.urihttp://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.publisherInstitute of Physics Publishing, Inc.
dc.relation.urihttp://iopscience.iop.org/0004-637X/776/2/68/
dc.titleDiscovery of an extended X-ray jet in AP librae
dc.typeJournal Article
dcterms.source.volume776
dcterms.source.number2
dcterms.source.startPage1
dcterms.source.endPage7
dcterms.source.issn0004-637X
dcterms.source.titleAstrophysical Journal
curtin.accessStatusFulltext not available


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