Mamon, 2 July 2005, PNe as astronomical tools, Gdansk Do planetary nebulae indicate Do planetary nebulae indicate a a lack of dark matter lack of dark matter in elliptical galaxies? in elliptical galaxies? with Avishai DEKEL (HU, Jerusalem), Felix STOEHR (IAP, Paris), TJ COX (Harvard), Greg NOVAK & Joel PRIMACK (UC Santa Cruz) Nature, accepted, astro-ph/0501622 Are PNe in ellipticals Are PNe in ellipticals young young ? ? and Ewa ŁOKAS (CAMK, Warsaw) MNRAS, submitted, astro-ph/0405491
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Do planetary nebulae indicate a lack of dark matter in elliptical galaxies?
Do planetary nebulae indicate a lack of dark matter in elliptical galaxies?. Are PNe in ellipticals young ?. with Avishai DEKEL ( HU, Jerusalem ), Felix STOEHR ( IAP, Paris ), TJ COX ( Harvard ), Greg NOVAK & Joel PRIMACK ( UC Santa Cruz ) Nature , accepted, astro-ph/0501622. and - PowerPoint PPT Presentation
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Gary Mamon, 2 July 2005, PNe as astronomical tools, Gdansk
Do planetary nebulae indicate Do planetary nebulae indicate a a lack of dark matterlack of dark matter in elliptical galaxies?in elliptical galaxies?
with
Avishai DEKEL (HU, Jerusalem), Felix STOEHR (IAP, Paris),TJ COX (Harvard), Greg NOVAK & Joel PRIMACK (UC Santa Cruz)Nature, accepted, astro-ph/0501622
Are PNe in ellipticals Are PNe in ellipticals youngyoung??
Gary Mamon, 2 July 2005, PNe as astronomical tools, Gdansk
Planetary Nebulae: Tracers at 1-3RPlanetary Nebulae: Tracers at 1-3Reffeff
N3379
[OIII]
5007 A
Gary Mamon, 2 July 2005, PNe as astronomical tools, Gdansk
PN velocity dispersions are lowPN velocity dispersions are low
Mendez et al. 01
N4697
Romanowsky et al. 03
DM
DM
DM
no DM
no DM
no DM
are Ellipticals naked?
Gary Mamon, 2 July 2005, PNe as astronomical tools, Gdansk
critical density Universe
universal M/L=387
log L/Lsun
log
(M/L
)/(M/L
sun)
Marinoni & Hudson 02
Predicted & observed M/LPredicted & observed M/L
Romanowsky et al 033
M/L = 33?
Gary Mamon, 2 July 2005, PNe as astronomical tools, Gdansk
1) Do ellipticals have normal 1) Do ellipticals have normal contents of dark matter?contents of dark matter?
ellipticals thought to be formed by mergers, mainly of spirals Toomre 77
Mamon 92, 00; Helsdon & Ponman 03Springel et al. 01; Lanzoni et al. 05
spirals have dark matter halos Sofue & Rubin 02
Gary Mamon, 2 July 2005, PNe as astronomical tools, Gdansk
Simulations of Simulations of major mergers of spiral galaxiesmajor mergers of spiral galaxies embedded in dark matter halos embedded in dark matter halos
Cox 04, PhD thesis
Gary Mamon, 2 July 2005, PNe as astronomical tools, Gdansk
Velocity dispersionsVelocity dispersions
no DM (R03)
with DM (R03)
DM
all starsyoung stars
Dekel et al 05
Gary Mamon, 2 July 2005, PNe as astronomical tools, Gdansk
2) What causes this discrepancy2) What causes this discrepancybetween between