Loooking for Arcs in the Spectra of J1819 385 - PowerPoint PPT Presentation

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Loooking for Arcs in the Spectra of J1819 385

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Loooking for Arcs in the Spectra of J1819 385. Barney Rickett, ... (RUG, ASTRON) S1(n,t) S2(fn,ft) pulsar. minutes. I = |E1 E2|2 if E1 and E2 are coherent: ... – PowerPoint PPT presentation

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Title: Loooking for Arcs in the Spectra of J1819 385


1
Loooking for Arcs in the Spectra of J1819385
  • Barney Rickett, Bill Coles
  • (UCSD)
  • J-P Macquart Ger de Bruyn
  • (RUG, ASTRON)

2
pulsar
minutes
S1(n,t)
S2(fn,ft)
3
scattering screen
I E1 E22 if E1 and E2 are coherent
E12 E22 2E1E2cos(Df) where Df
2p(n1t1-n2t2) t1 tdt1 , n1 ndn1 Df
2pn(dt1- dt2)(dn1- dn2)t .. ..O(dn dt)
V
dt1 zq12/2c is the relative time delay dn1
n(V.q1)/c is the relative Doppler frequency
(ie fringe frequency)
4
fn dt1- dt2 q12- q12 (z/2c) relative
delay ft dn1- dn2 (q1x- q2x)V/l fringe
frequency
With q2 0 we get q1x ft l/V and q12
2cfn/z so q1y (2cfn/z - (ft l/V)2 Then
S2(fn, ft) is bounded by a parabolic "arc" fn
ft2 zl2/2cV2
5
quasar
D
qsrc
Coherence scale at the screen bsrc l/(pqsrc)
s
ISM
z
At spacing s, relative time delay fn
s2/(2cz) Fringe amplitude (S2) is decreased due
to loss of coherence at fn gt bsrc2/(2cz)
l2/(2p2zcq2src) ie fn gt (qFr/qsrc)2(1/2pn0) This
gives a cut-off in delay due to source diameter
observer
6
Simulation of screen at 1.4 GHz with 160 MHz
total Bandwidth
7
Simulation of screen at 1.4 GHz with 160 MHz
total Bandwidth
8
Simulation of screen at 1.4 GHz with 160 MHz
total Bandwidth
9
Simulation of screen at 1.4 GHz with 160 MHz
total Bandwidth
10
Now look at 1.4 GHz observations of
J1819385 From Westerbork 22 Feb 2003 12 Apr
2003 19 Jun 2003 25 Dec 2003
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  • Screen Model
  • Distance Lpc
  • Isotropic Kolmogorov spectrum (zero inner
    scale)
  • qFr 25µas (LpcnGHz)-0.5
  • ntrans 5 GHz to match large scintillation
    index at 5 GHz
  • Source Model Two Gaussian components
  • L 5 pc 50 pc
  • Angular radius 0.03 qFr qa 4.7 1.5 µas
    (FWHM)
  • Angular radius qFr qb 160 50 µas (FWHM)
  • Ratio of flux densities is parameter in
    following simulations..

17
0.03 qFr 10 Flux qFr 90 Flux
18
0.03 qFr 5 Flux qFr 95 Flux
19
0.03 qFr 1 Flux qFr 99 Flux
20
5pc, 50pc at 50 km/s
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Preliminary Results (work in progress)
  • No arc detected at 21 or 6 cm (need to set
    detection threshold)
  • Screen model at 5-50 pc ultra-compact (1-5 µas)
    component has less than 1 mJy at 21 cm
  • gt Tb lt 1.5x1013 K
  • OR
  • inner scale gt 200-500 km
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