Multiwavelength study of Cygnus A II. X-ray inverse-Compton emission from a relic counterjet and implications for jet duty-cycles
The duty-cycle of powerful radio galaxies and quasars such as the prototype Cygnus A is poorly understood. X-ray observations of inverse-Compton scattered Cosmic Microwave Background (ICCMB) photons probe lower Lorentz-factor particles than radio observations of synchrotron emission. Comparative stu...
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| Format: | Journal article |
| Language: | English |
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2008
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| _version_ | 1797071576419532800 |
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| author | Steenbrugge, K Blundell, K Duffy, P |
| author_facet | Steenbrugge, K Blundell, K Duffy, P |
| author_sort | Steenbrugge, K |
| collection | OXFORD |
| description | The duty-cycle of powerful radio galaxies and quasars such as the prototype Cygnus A is poorly understood. X-ray observations of inverse-Compton scattered Cosmic Microwave Background (ICCMB) photons probe lower Lorentz-factor particles than radio observations of synchrotron emission. Comparative studies of the nearer and further lobes, separated by many 10s of kpc and thus 10s of thousands of years in light-travel time, yield additional temporal resolution in studies of the lifecycles. We have co-added all archival Chandra ACIS-I data and present a deep 200 ks image of Cygnus A. This deep image reveals the presence of X-ray emission from a counterjet i.e. a jet receding from Earth and related to a previous episode of jet activity. The non-thermal X-ray emission, we interpret as ICCMB radiation. There is an absence of any discernible X-ray emission associated with a jet flowing towards Earth. We conclude that: (1) The emission from a relic jet, indicates a previous episode of jet activity, that took place earlier than the current jet activity appearing as synchrotron radio emission. (2) The presence of X-ray emission from a relic counterjet of Cygnus A and the absence of X-ray emission associated with any relic approaching jet constrains the timescale between successive episodes of jet activity to ~10^6 years. (3) Transverse expansion of the jet causes expansion losses which shifts the energy distribution to lower energies. (4) Assuming the electrons cooled due to adiabatic expansion, the required magnetic field strength is substantially smaller than the equipartition magnetic field strength. (5) A high minimum Lorentz factor for the distribution of relativistic particles in the current jet, of a few 10^3, is ejected from the central nucleus of this active galaxy. Abridged. |
| first_indexed | 2024-03-06T22:55:18Z |
| format | Journal article |
| id | oxford-uuid:602941ba-0aae-4afb-ab44-41549a11058d |
| institution | University of Oxford |
| language | English |
| last_indexed | 2024-03-06T22:55:18Z |
| publishDate | 2008 |
| record_format | dspace |
| spelling | oxford-uuid:602941ba-0aae-4afb-ab44-41549a11058d2022-03-26T17:51:40ZMultiwavelength study of Cygnus A II. X-ray inverse-Compton emission from a relic counterjet and implications for jet duty-cyclesJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:602941ba-0aae-4afb-ab44-41549a11058dEnglishSymplectic Elements at Oxford2008Steenbrugge, KBlundell, KDuffy, PThe duty-cycle of powerful radio galaxies and quasars such as the prototype Cygnus A is poorly understood. X-ray observations of inverse-Compton scattered Cosmic Microwave Background (ICCMB) photons probe lower Lorentz-factor particles than radio observations of synchrotron emission. Comparative studies of the nearer and further lobes, separated by many 10s of kpc and thus 10s of thousands of years in light-travel time, yield additional temporal resolution in studies of the lifecycles. We have co-added all archival Chandra ACIS-I data and present a deep 200 ks image of Cygnus A. This deep image reveals the presence of X-ray emission from a counterjet i.e. a jet receding from Earth and related to a previous episode of jet activity. The non-thermal X-ray emission, we interpret as ICCMB radiation. There is an absence of any discernible X-ray emission associated with a jet flowing towards Earth. We conclude that: (1) The emission from a relic jet, indicates a previous episode of jet activity, that took place earlier than the current jet activity appearing as synchrotron radio emission. (2) The presence of X-ray emission from a relic counterjet of Cygnus A and the absence of X-ray emission associated with any relic approaching jet constrains the timescale between successive episodes of jet activity to ~10^6 years. (3) Transverse expansion of the jet causes expansion losses which shifts the energy distribution to lower energies. (4) Assuming the electrons cooled due to adiabatic expansion, the required magnetic field strength is substantially smaller than the equipartition magnetic field strength. (5) A high minimum Lorentz factor for the distribution of relativistic particles in the current jet, of a few 10^3, is ejected from the central nucleus of this active galaxy. Abridged. |
| spellingShingle | Steenbrugge, K Blundell, K Duffy, P Multiwavelength study of Cygnus A II. X-ray inverse-Compton emission from a relic counterjet and implications for jet duty-cycles |
| title | Multiwavelength study of Cygnus A II. X-ray inverse-Compton emission
from a relic counterjet and implications for jet duty-cycles |
| title_full | Multiwavelength study of Cygnus A II. X-ray inverse-Compton emission
from a relic counterjet and implications for jet duty-cycles |
| title_fullStr | Multiwavelength study of Cygnus A II. X-ray inverse-Compton emission
from a relic counterjet and implications for jet duty-cycles |
| title_full_unstemmed | Multiwavelength study of Cygnus A II. X-ray inverse-Compton emission
from a relic counterjet and implications for jet duty-cycles |
| title_short | Multiwavelength study of Cygnus A II. X-ray inverse-Compton emission
from a relic counterjet and implications for jet duty-cycles |
| title_sort | multiwavelength study of cygnus a ii x ray inverse compton emission from a relic counterjet and implications for jet duty cycles |
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