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Intrinsic structure and kinematics of the sub-parsec scale jet of M87

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Presentation on theme: "Intrinsic structure and kinematics of the sub-parsec scale jet of M87"— Presentation transcript:

1 Intrinsic structure and kinematics of the sub-parsec scale jet of M87
Y. Y. Kovalev MPIfR-Bonn; ASC Lebedev Alaska May 22, 2007

2 Collaborators Y. Y. Kovalev (MPIfR-Bonn, ASC Lebedev)
K. I. Kellermann (NRAO) M. L. Lister (Purdue University) D. C. Homan (Denison University) A. P. Lobanov(MPIfR-Bonn) 2 cm VLBA / MOJAVE group Alaska May 22, 2007 Arecibo Observatory Library Colloquium

3 Sub-parsec-scale jet in M87 at 15 GHz
Alaska May 22, 2007

4 3 mas long “Counter-jet”
15 GHz Ly et al. (2007) Alaska May 22, 2007

5 Counter-jet tests: is it real or an imaging artifact?
Deep VLBA+VLA M87 image A model without a counter-jet was used to produce the fake uv dataset 1: no counter-jet is detected in the image A model with a counter-jet was used to produce the fake uv dataset 2: the counter-jet detected in the image Alaska May 22, 2007

6 M87 CP results: -0.5% Homan & Lister (2006) Alaska May 22, 2007

7 Negative speed of a counter-jet feature
Alaska May 22, 2007

8 Intrinsic jet structure
Alaska May 22, 2007

9 Intrinsic structure of the counter jet
Alaska May 22, 2007

10 15 GHz VLBA M87 movie Alaska May 22, 2007

11 Kinematics Alaska Fastest jet speed: 0.03c Counter-jet: -0.01c
May 22, 2007

12 Discussion Large scale jet opening angle: 6 degrees.
Linear polarization data corrected for FRM from Zavala & Taylor (2002) suggest highly ordered longitudinal magnetic field. We argue that the “counter-jet” is the counter-jet. Jet / Counter-jet brightness ratio is measured to be 14. Assuming viewing angle degrees, this brightness ratio suggests that the bulk flow is ( )c. If the edge brightened jet structure is due to a velocity gradient and the jet is described by a two component model with a fast spine and a slow sheath, this could explain the detected variable TeV emission from M87 (Aharonian et al. 2006) following the spine-sheath model of Ghisellini et al. (2005). Alaska May 22, 2007

13 Thank you June 10, 2005 April 11, 2005 NASA GSFC
Arecibo Observatory Library Colloquium


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