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Detailed structure of the X-ray jet in 4C 19.44 (PKS1354+195). / Schwartz, D. A.; Harris, D. E.; Landt, H.; Siemiginowska, A.; Perlman, E. S.; Cheung, C. C.; Gelbord, J. M.; Worrall, D. M.; Birkinshaw, M.; Jorstad, S. G.; Marscher, A. P.; Stawarz, L.

In: Proceedings of the International Astronomical Union, Vol. 2, No. S238, 08.2006, p. 443-444.

Research output: Contribution to journal › Article

Harvard

Schwartz, DA, Harris, DE, Landt, H, Siemiginowska, A, Perlman, ES, Cheung, CC, Gelbord, JM, Worrall, DM, Birkinshaw, M, Jorstad, SG, Marscher, AP & Stawarz, L 2006, 'Detailed structure of the X-ray jet in 4C 19.44 (PKS1354+195)', Proceedings of the International Astronomical Union, vol. 2, no. S238, pp. 443-444. https://doi.org/10.1017/S1743921307005868

APA

Schwartz, D. A., Harris, D. E., Landt, H., Siemiginowska, A., Perlman, E. S., Cheung, C. C., Gelbord, J. M., Worrall, D. M., Birkinshaw, M., Jorstad, S. G., Marscher, A. P., & Stawarz, L. (2006). Detailed structure of the X-ray jet in 4C 19.44 (PKS1354+195). Proceedings of the International Astronomical Union, 2(S238), 443-444. https://doi.org/10.1017/S1743921307005868

Vancouver

Schwartz DA, Harris DE, Landt H, Siemiginowska A, Perlman ES, Cheung CC et al. Detailed structure of the X-ray jet in 4C 19.44 (PKS1354+195). Proceedings of the International Astronomical Union. 2006 Aug;2(S238):443-444. https://doi.org/10.1017/S1743921307005868

Author

Schwartz, D. A. ; Harris, D. E. ; Landt, H. ; Siemiginowska, A. ; Perlman, E. S. ; Cheung, C. C. ; Gelbord, J. M. ; Worrall, D. M. ; Birkinshaw, M. ; Jorstad, S. G. ; Marscher, A. P. ; Stawarz, L. / Detailed structure of the X-ray jet in 4C 19.44 (PKS1354+195). In: Proceedings of the International Astronomical Union. 2006 ; Vol. 2, No. S238. pp. 443-444.

BibTeX

@article{c34f84ca62b74d868466d2a7fb280ce2,
title = "Detailed structure of the X-ray jet in 4C 19.44 (PKS1354+195)",
abstract = "We investigate the variations of the magnetic field, Doppler factor, and relativistic particle density along the jet of a quasar at z=0.72. We chose 4C 19.44 for this study because of its length and straight morphology. The 18 arcsec length of the jet provides many independent resolution elements in the Chandra X-ray image. The straightness suggests that geometry factors, although uncertain, are almost constant along the jet. We assume the X-ray emission is from inverse Compton scattering of the cosmic microwave background. With the aid of assumptions about jet alignment, equipartition between magnetic-field and relativistic-particle energy, and filling factors, we find that the jet is in bulk relativistic motion with a Doppler factor 6 at an angle no more than 10 to the line of sight over de-projected distances 150600 kpc from the quasar, and with a magnetic field 10 Gauss.",
keywords = "(Galaxies:) quasars: individual (4C 19.44, PKS 1354+135), Galaxies: jets, X-rays",
author = "Schwartz, {D. A.} and Harris, {D. E.} and H. Landt and A. Siemiginowska and Perlman, {E. S.} and Cheung, {C. C.} and Gelbord, {J. M.} and Worrall, {D. M.} and M. Birkinshaw and Jorstad, {S. G.} and Marscher, {A. P.} and L. Stawarz",
note = "Funding Information: We acknowledge support of NASA contract NAS8 39073 to SAO, CXC grants GO5-6116B, GO6-7111A, GO6-7111B, and HST grant HST-GO-10762.01-A.",
year = "2006",
month = aug,
doi = "10.1017/S1743921307005868",
language = "English",
volume = "2",
pages = "443--444",
journal = "Proceedings of the International Astronomical Union",
issn = "1743-9213",
publisher = "Cambridge University Press",
number = "S238",

}

RIS

TY - JOUR

T1 - Detailed structure of the X-ray jet in 4C 19.44 (PKS1354+195)

AU - Schwartz, D. A.

AU - Harris, D. E.

AU - Landt, H.

AU - Siemiginowska, A.

AU - Perlman, E. S.

AU - Cheung, C. C.

AU - Gelbord, J. M.

AU - Worrall, D. M.

AU - Birkinshaw, M.

AU - Jorstad, S. G.

AU - Marscher, A. P.

AU - Stawarz, L.

N1 - Funding Information: We acknowledge support of NASA contract NAS8 39073 to SAO, CXC grants GO5-6116B, GO6-7111A, GO6-7111B, and HST grant HST-GO-10762.01-A.

PY - 2006/8

Y1 - 2006/8

N2 - We investigate the variations of the magnetic field, Doppler factor, and relativistic particle density along the jet of a quasar at z=0.72. We chose 4C 19.44 for this study because of its length and straight morphology. The 18 arcsec length of the jet provides many independent resolution elements in the Chandra X-ray image. The straightness suggests that geometry factors, although uncertain, are almost constant along the jet. We assume the X-ray emission is from inverse Compton scattering of the cosmic microwave background. With the aid of assumptions about jet alignment, equipartition between magnetic-field and relativistic-particle energy, and filling factors, we find that the jet is in bulk relativistic motion with a Doppler factor 6 at an angle no more than 10 to the line of sight over de-projected distances 150600 kpc from the quasar, and with a magnetic field 10 Gauss.

AB - We investigate the variations of the magnetic field, Doppler factor, and relativistic particle density along the jet of a quasar at z=0.72. We chose 4C 19.44 for this study because of its length and straight morphology. The 18 arcsec length of the jet provides many independent resolution elements in the Chandra X-ray image. The straightness suggests that geometry factors, although uncertain, are almost constant along the jet. We assume the X-ray emission is from inverse Compton scattering of the cosmic microwave background. With the aid of assumptions about jet alignment, equipartition between magnetic-field and relativistic-particle energy, and filling factors, we find that the jet is in bulk relativistic motion with a Doppler factor 6 at an angle no more than 10 to the line of sight over de-projected distances 150600 kpc from the quasar, and with a magnetic field 10 Gauss.

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

KW - Galaxies: jets

KW - X-rays

UR - http://www.scopus.com/inward/record.url?scp=37049028818&partnerID=8YFLogxK

U2 - 10.1017/S1743921307005868

DO - 10.1017/S1743921307005868

M3 - Article

AN - SCOPUS:37049028818

VL - 2

SP - 443

EP - 444

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

SN - 1743-9213

IS - S238

ER -

ID: 88374463