The X-ray jet and lobes of PKS 1354+195 (=4C 19.44)

D. A. Schwartz; D. E. Harris; H. Landt; A. Siemiginowska; H. L. Marshall; J. M. Gelbord; E. S. Perlman; M. Georganopoulos; M. Birkinshaw; D. M. Worrall; C. C. Cheung; L. Stawarz; S. G. Jorstad; A. P. Marscher; Y. Uchiyama; C. M. Urry

doi:10.1007/s10509-007-9548-y

The X-ray jet and lobes of PKS 1354+195 (=4C 19.44)

D. A. Schwartz^*, D. E. Harris, H. Landt, A. Siemiginowska, H. L. Marshall, J. M. Gelbord, E. S. Perlman, M. Georganopoulos, M. Birkinshaw, D. M. Worrall, C. C. Cheung, L. Stawarz, S. G. Jorstad, A. P. Marscher, Y. Uchiyama, C. M. Urry

^*Corresponding author for this work

School of Physics

Research output: Contribution to journal › Article (Academic Journal) › peer-review

7 Citations (Scopus)

Abstract

We present a Chandra image of the quasar, jet, and lobes of PKS 1354+195 (=4C 19.44). The radio jet is 18 arcsec long, and appears to be very straight. The length gives many independent spatial resolution elements in the Chandra image while the straightness implies that the geometrical factors are constant along the jet although their values are uncertain. We also have 4 frequency radio images with half to one arcsecond angular resolution, and use HST and Spitzer data to study the broad band spectral energy distributions. The X-ray and radio spectra are both consistent with a spectrum f(nu) alpha nu(-0.7) stop for the integrated jet. Using that spectral index, the model of inverse Compton scattering of electrons on the cosmic microwave background (IC/CMB) gives magnetic field strengths and Doppler factors that are relatively constant along the jet. Extended X-ray emission is evident in the direction of the otherwise unseen counter-jet. X-ray emission continues past the radio jet to the South, and is detected within both the southern and northern radio lobes.

Original language	English
Pages (from-to)	341-345
Number of pages	5
Journal	Astrophysics & Space Science
Volume	311
Issue number	1-3
DOIs	https://doi.org/10.1007/s10509-007-9548-y
Publication status	Published - Oct 2007
Event	5th Stromlo Symposium on Disks, Winds and Jets - From Planets to Quasars - Canberra, Australia Duration: 3 Dec 2006 → 8 Dec 2006

Keywords

(Galaxies : ) quasars : individual (4C 19.44, PKS 1354+135)
galaxies : jets
X-rays : individual (4C 19.44, PKS 1354+135)
radio continuum : general
magnetic fields
ACTIVE GALACTIC NUCLEI
HUBBLE-SPACE-TELESCOPE
EXTENDED RADIO JETS
CHANDRA OBSERVATIONS
OBJECTS

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Schwartz, D. A., Harris, D. E., Landt, H., Siemiginowska, A., Marshall, H. L., Gelbord, J. M., Perlman, E. S., Georganopoulos, M., Birkinshaw, M., Worrall, D. M., Cheung, C. C., Stawarz, L., Jorstad, S. G., Marscher, A. P., Uchiyama, Y., & Urry, C. M. (2007). The X-ray jet and lobes of PKS 1354+195 (=4C 19.44). Astrophysics & Space Science, 311(1-3), 341-345. https://doi.org/10.1007/s10509-007-9548-y

Schwartz, D. A. ; Harris, D. E. ; Landt, H. ; Siemiginowska, A. ; Marshall, H. L. ; Gelbord, J. M. ; Perlman, E. S. ; Georganopoulos, M. ; Birkinshaw, M. ; Worrall, D. M. ; Cheung, C. C. ; Stawarz, L. ; Jorstad, S. G. ; Marscher, A. P. ; Uchiyama, Y. ; Urry, C. M. / The X-ray jet and lobes of PKS 1354+195 (=4C 19.44). In: Astrophysics & Space Science. 2007 ; Vol. 311, No. 1-3. pp. 341-345.

@article{7b72db3b450f4e49a2a8f4a77296371b,

title = "The X-ray jet and lobes of PKS 1354+195 (=4C 19.44)",

abstract = "We present a Chandra image of the quasar, jet, and lobes of PKS 1354+195 (=4C 19.44). The radio jet is 18 arcsec long, and appears to be very straight. The length gives many independent spatial resolution elements in the Chandra image while the straightness implies that the geometrical factors are constant along the jet although their values are uncertain. We also have 4 frequency radio images with half to one arcsecond angular resolution, and use HST and Spitzer data to study the broad band spectral energy distributions. The X-ray and radio spectra are both consistent with a spectrum f(nu) alpha nu(-0.7) stop for the integrated jet. Using that spectral index, the model of inverse Compton scattering of electrons on the cosmic microwave background (IC/CMB) gives magnetic field strengths and Doppler factors that are relatively constant along the jet. Extended X-ray emission is evident in the direction of the otherwise unseen counter-jet. X-ray emission continues past the radio jet to the South, and is detected within both the southern and northern radio lobes.",

keywords = "(Galaxies : ) quasars : individual (4C 19.44, PKS 1354+135), galaxies : jets, X-rays : individual (4C 19.44, PKS 1354+135), radio continuum : general, magnetic fields, ACTIVE GALACTIC NUCLEI, HUBBLE-SPACE-TELESCOPE, EXTENDED RADIO JETS, CHANDRA OBSERVATIONS, OBJECTS",

author = "Schwartz, {D. A.} and Harris, {D. E.} and H. Landt and A. Siemiginowska and Marshall, {H. L.} and Gelbord, {J. M.} and Perlman, {E. S.} and M. Georganopoulos and M. Birkinshaw and Worrall, {D. M.} and Cheung, {C. C.} and L. Stawarz and Jorstad, {S. G.} and Marscher, {A. P.} and Y. Uchiyama and Urry, {C. M.}",

year = "2007",

month = oct,

doi = "10.1007/s10509-007-9548-y",

language = "English",

volume = "311",

pages = "341--345",

journal = "Astrophysics & Space Science",

issn = "0004-640X",

publisher = "Springer Netherlands",

number = "1-3",

note = "5th Stromlo Symposium on Disks, Winds and Jets - From Planets to Quasars ; Conference date: 03-12-2006 Through 08-12-2006",

}

Schwartz, DA, Harris, DE, Landt, H, Siemiginowska, A, Marshall, HL, Gelbord, JM, Perlman, ES, Georganopoulos, M, Birkinshaw, M , Worrall, DM, Cheung, CC, Stawarz, L, Jorstad, SG, Marscher, AP, Uchiyama, Y & Urry, CM 2007, 'The X-ray jet and lobes of PKS 1354+195 (=4C 19.44)', Astrophysics & Space Science, vol. 311, no. 1-3, pp. 341-345. https://doi.org/10.1007/s10509-007-9548-y

The X-ray jet and lobes of PKS 1354+195 (=4C 19.44). / Schwartz, D. A.; Harris, D. E.; Landt, H.; Siemiginowska, A.; Marshall, H. L.; Gelbord, J. M.; Perlman, E. S.; Georganopoulos, M.; Birkinshaw, M.; Worrall, D. M.; Cheung, C. C.; Stawarz, L.; Jorstad, S. G.; Marscher, A. P.; Uchiyama, Y.; Urry, C. M.

In: Astrophysics & Space Science, Vol. 311, No. 1-3, 10.2007, p. 341-345.

Research output: Contribution to journal › Article (Academic Journal) › peer-review

TY - JOUR

T1 - The X-ray jet and lobes of PKS 1354+195 (=4C 19.44)

AU - Schwartz, D. A.

AU - Harris, D. E.

AU - Landt, H.

AU - Siemiginowska, A.

AU - Marshall, H. L.

AU - Gelbord, J. M.

AU - Perlman, E. S.

AU - Georganopoulos, M.

AU - Birkinshaw, M.

AU - Worrall, D. M.

AU - Cheung, C. C.

AU - Stawarz, L.

AU - Jorstad, S. G.

AU - Marscher, A. P.

AU - Uchiyama, Y.

AU - Urry, C. M.

PY - 2007/10

Y1 - 2007/10

N2 - We present a Chandra image of the quasar, jet, and lobes of PKS 1354+195 (=4C 19.44). The radio jet is 18 arcsec long, and appears to be very straight. The length gives many independent spatial resolution elements in the Chandra image while the straightness implies that the geometrical factors are constant along the jet although their values are uncertain. We also have 4 frequency radio images with half to one arcsecond angular resolution, and use HST and Spitzer data to study the broad band spectral energy distributions. The X-ray and radio spectra are both consistent with a spectrum f(nu) alpha nu(-0.7) stop for the integrated jet. Using that spectral index, the model of inverse Compton scattering of electrons on the cosmic microwave background (IC/CMB) gives magnetic field strengths and Doppler factors that are relatively constant along the jet. Extended X-ray emission is evident in the direction of the otherwise unseen counter-jet. X-ray emission continues past the radio jet to the South, and is detected within both the southern and northern radio lobes.

AB - We present a Chandra image of the quasar, jet, and lobes of PKS 1354+195 (=4C 19.44). The radio jet is 18 arcsec long, and appears to be very straight. The length gives many independent spatial resolution elements in the Chandra image while the straightness implies that the geometrical factors are constant along the jet although their values are uncertain. We also have 4 frequency radio images with half to one arcsecond angular resolution, and use HST and Spitzer data to study the broad band spectral energy distributions. The X-ray and radio spectra are both consistent with a spectrum f(nu) alpha nu(-0.7) stop for the integrated jet. Using that spectral index, the model of inverse Compton scattering of electrons on the cosmic microwave background (IC/CMB) gives magnetic field strengths and Doppler factors that are relatively constant along the jet. Extended X-ray emission is evident in the direction of the otherwise unseen counter-jet. X-ray emission continues past the radio jet to the South, and is detected within both the southern and northern radio lobes.

KW - (Galaxies : ) quasars : individual (4C 19.44, PKS 1354+135)

KW - galaxies : jets

KW - X-rays : individual (4C 19.44, PKS 1354+135)

KW - radio continuum : general

KW - magnetic fields

KW - ACTIVE GALACTIC NUCLEI

KW - HUBBLE-SPACE-TELESCOPE

KW - EXTENDED RADIO JETS

KW - CHANDRA OBSERVATIONS

KW - OBJECTS

U2 - 10.1007/s10509-007-9548-y

DO - 10.1007/s10509-007-9548-y

M3 - Article (Academic Journal)

VL - 311

SP - 341

EP - 345

JO - Astrophysics & Space Science

JF - Astrophysics & Space Science

SN - 0004-640X

IS - 1-3

T2 - 5th Stromlo Symposium on Disks, Winds and Jets - From Planets to Quasars

Y2 - 3 December 2006 through 8 December 2006

ER -

The X-ray jet and lobes of PKS 1354+195 (=4C 19.44)

Abstract

Keywords

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