Predicting analytically stripped and re-accreted mass fraction - - PowerPoint PPT Presentation

predicting analytically stripped and re accreted mass
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Predicting analytically stripped and re-accreted mass fraction - - PowerPoint PPT Presentation

Predicting analytically stripped and re-accreted mass fraction Joachim Kppen A gas parcel in the galactic disk potential Restoring force Gunn & Gott criterion = force acting slowly escape potential Restoring force What happens


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Predicting ‘analytically’ stripped and re-accreted mass fraction

Joachim Köppen

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A gas parcel in the galactic disk

potential Restoring force

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Gunn & Gott criterion

potential Restoring force = force acting slowly escape

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What happens after a short force pulse?

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Taking RPS as a collision

  • Momentum balance

ΣISM * vAFTER = ΣICM * vICM

  • Stripping if

vAFTER > vESC

  • Works well to explain stripped mass

fractions in Pavel’s SPH models

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How to predict the re-accretable fraction?

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Simulations with test particle models

stripped (ETOTAL > 0) kicked above 1 kpc unmoved At time of max. pressure

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Remember the ballistic galvanometer?

  • If an undamped harmonic oscillator is

kicked by a pulse shorter than its natural period, it will oscillate with an amplitude which is proportional to the time-integrated force i.e. the momentum transferred to it. NB: The amplitude is independent of the form of the pulse.

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Period of vertical oscillations

Pavel’s « standard » run 10 Myr

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Let’s apply it to face-on RPS

  • Equation of motion

d(ΣISMv)/dt = ρICM (vICM-v)² - ΣISM dΦ/dz

  • Solution: (a) during the kick (z = v = 0)

ΣISMvAFTER = ρICM vICM² Δt

  • Solution: (b) after the kick (Force=0; v = vAFTER)

d(ΣISMv)/dt = - ΣISM dΦ/dz  (harmonic) oscillation with amplitude corresponding to initial kick …

  • the important parameter:

ρICM vICM² Δt = vICM (ρICM vICM Δt) = vICM ΣICM

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Given the speed after the kick

  • … and the potential, we can compute how

high above the disk the gas packet can move

  • … and hence we can predict which parts
  • f the disk will be displaced by some

minimum height, say 1 kpc

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We get

stripped kicked above 1kpc but not stripped R [kpc] stays in disk

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Compare with Pavel’s SPH models

Not all kicked matter really reaches above 1 kpc …

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… while other matter is displaced Depending on the initial vertical velocity some kicked matter remains unmoved

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Summary

  • Momentum transfer determines the fate of

a gas parcel

  • The primary parameter is the column

density ΣICM of the accumulated ICM

  • For the reaccreted fraction we can give
  • nly an upper limit
  • For slow stripping, the efficiency of

momentum transfer will be less!