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dc.contributor.authorMingo, B.
dc.contributor.authorHardcastle, M.J.
dc.contributor.authorCroston, J.H.
dc.contributor.authorEvans, D.A.
dc.contributor.authorKraft, R.P.
dc.contributor.authorKharb, P.
dc.contributor.authorLenc, E.
dc.date.accessioned2013-06-17T12:45:44Z
dc.date.available2013-06-17T12:45:44Z
dc.date.issued2012-10-20
dc.identifier.citationMingo , B , Hardcastle , M J , Croston , J H , Evans , D A , Kraft , R P , Kharb , P & Lenc , E 2012 , ' Shocks, seyferts, and the supernova remnant connection : A chandra observation of the circinus galaxy ' The Astrophysical Journal , vol. 758 , no. 2 , 95 . https://doi.org/10.1088/0004-637X/758/2/95
dc.identifier.issn0004-637X
dc.identifier.otherPURE: 1911478
dc.identifier.otherPURE UUID: efa4fbe5-8a55-463a-a177-232c07d96e50
dc.identifier.otherScopus: 84867302482
dc.identifier.urihttp://hdl.handle.net/2299/10787
dc.descriptionCopyright American Astronomical Society
dc.description.abstractWe analyze new Chandra observations of the nearest (D = 4 Mpc) Seyfert 2 active galaxy, Circinus, and match them to pre-existing radio, infrared, and optical data to study the kpc-scale emission. The proximity of Circinus allows us to observe in striking detail the structure of the radio lobes, revealing for the first time edge-brightened emission in both X-rays and radio. After considering various other possible scenarios, we show that this extended emission in Circinus is most likely caused by a jet-driven outflow, which is driving shells of strongly shocked gas into the halo of the host galaxy. In this context, we estimate Mach numbers -3.6 and -5.3 for the W and E shells, respectively. We derive temperatures of 0.74 keV and 0.8-1.8 keV for the W and E shells and an expansion velocity of ∼900-950kms . We estimate that the total energy (thermal and kinetic) involved in creating both shells is ∼2 × ∼10 erg, and their age is 10 yr. Comparing these results with those we previously obtained for Centaurus A, NGC3801, and Mrk 6, we show that these parameters scale approximately with the radio power of the parent active galactic nucleus (AGN). The spatial coincidence between the X-ray and edge-brightened radio emission in Circinus resembles the morphology of some supernova remnant shocks. This parallel has been expected for AGNs but has never been observed before. We investigate what underlying mechanisms both types of systems may have in common, arguing that, in Circinus, the edge-brightening in the shells may be accounted for by a B field enhancement caused by shock compression but do not preclude some local particle acceleration. These results can be extrapolated to other low-power systems, particularly those with late-type hosts.en
dc.language.isoeng
dc.relation.ispartofThe Astrophysical Journal
dc.rights/dk/atira/pure/core/openaccesspermission/open
dc.titleShocks, seyferts, and the supernova remnant connection : A chandra observation of the circinus galaxyen
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.description.statusPeer reviewed
dc.identifier.urlhttp://www.scopus.com/inward/record.url?scp=84867302482&partnerID=8YFLogxK
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dc.description.versiontypeSubmitted Version
rioxxterms.versionSMUR
rioxxterms.versionofrecordhttps://doi.org/10.1088/0004-637X/758/2/95
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstyperestrictedAccess


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