A simple model for superluminal motion and state transition of microquasars
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A simple model for superluminal motion and state transition of microquasars. Huazhong University of Science and technology. Gong Biping. Bulk motion. M. Rees 1966. Mirabel et al., 1994, Nature, 371, 46. XTE J1550-564 in 2000 and 2002. 2002, Science, 298, 196. GRS 1915+105

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A simple model for superluminal motion and state transition of microquasars

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A simple model for superluminal motion and state transition of microquasars

A simple model for superluminal motion and state transition of microquasars

Huazhong University of Science and technology

Gong Biping


Bulk motion

Bulk motion

M. Rees 1966


A simple model for superluminal motion and state transition of microquasars

Mirabel et al., 1994, Nature, 371, 46.


Xte j1550 564 in 2000 and 2002

XTE J1550-564 in 2000 and 2002

2002, Science, 298, 196.


A simple model for superluminal motion and state transition of microquasars

GRS 1915+105

in 1994 and 1997

2004, ARA&A, 42, 317.


A simple model for superluminal motion and state transition of microquasars

Miller-Jones et al

2005


Position angle variation

Position angle variation

1999, ApJ, 511, 398.


Difficult questions on slm

Difficult questions on SLM

(a) why the ratio of the displacement of the approaching blob to the receding blob is not a constant.

(b) why the receding jet appears later than the approaching jet in XTEJ1550-564 (for months) and GRS 1915+105 (for days).

(c) why deceleration appeared in XTE J1550-564 but not in GRS 1915+105.

(d) why the position angle changes 10 deg in 20-30 days in GRS 1915+105.

(e) why there is obvious oscillation in the receding blob.

(f) why 20% discrepancy in proper motion between the ejection of 1994 and 1997.

(g) why the size of condensations do not increase rapidly as expected from adiabatic expansion.


Other possibility

Other possibility?

Bulk motion

precession


The precession of grs 1915 105 and ss433

The precession of GRS 1915+105 and SS433


Jet precession model

Jet precession model


Primary precession

Primary precession


Perturbation to orbital elements

Perturbation to orbital elements


Nutation

Nutation


Slm under precession scenario

SLM under precession scenario


A simple model for superluminal motion and state transition of microquasars

(a) why the ratio of the displacement of the approaching blob to the receding blob is not a constant.

is not a constant under precession model

It is a constant under bulk motion


A simple model for superluminal motion and state transition of microquasars

(b) why the receding jet appears later than the approaching jet in XTEJ1550-564 .


A simple model for superluminal motion and state transition of microquasars

(c) why deceleration appeared in XTE J1550-564 but not in GRS 1915+105.


A simple model for superluminal motion and state transition of microquasars

(d) why the decrease in flux density with angular separation from the core on GRS 1915+105 is remarkably similar with that of SS 433.

(e) why 20% discrepancy in proper motion between the ejection of 1994 and 1997.


A simple model for superluminal motion and state transition of microquasars

(f) why the position angle changes 10 deg in 20-30 days in GRS 1915+105.

(g) why there is obvious oscillation in the receding blob.


A simple model for superluminal motion and state transition of microquasars

Observations which are difficult to understand

under the bulk motion scenario can be interpreted

by the jet precession model naturally.


The state evolution of grs 1915 105

The state evolution of GRS 1915+105

Fender et al. 2004


A simple model for superluminal motion and state transition of microquasars

Fender et al. 2004


A simple model for superluminal motion and state transition of microquasars

Structured jet


Precession of the structured jet

Precession of the structured jet


Summary

Summary

Simple

Unified

Easy to test


A simple model for superluminal motion and state transition of microquasars

Thanks for your attention


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