Title: Hypervelocity Stars Ejected from the Galactic Center
1Hypervelocity StarsEjected from the Galactic
Center
MMT Symposium June 14, 2006 Warren R.
Brown Harvard-Smithsonian CfA Collaborators
Margaret Geller, Scott Kenyon, Michael Kurtz
2The Milky Way
30 kpc
8 kpc
r100 kpc
Kaufmann
3The Galactic Center
http//www.mpe.mpg.de/ir/GC/prop.html
4Eisenhauer et al. 2005
5Three-body exchange
Bromley 2005
6Radial Velocities from the MMT
7(No Transcript)
8An Unexpected Star
Brown et al. (2005)
- VRF 709 km/s
- B9 main sequence star.
- Fe/H 0.
- Distance 110 kpc.
- Travel time 160 Myr to 110 kpc.
9A Hypervelocity Star
Brown et al. (2005)
- VRF 709 km/s
- B9 main sequence star.
- Fe/H 0.
- Distance 110 kpc.
- Travel time 160 Myr to 110 kpc.
NY Times
10Our Search for more Hypervelocity Stars
O
B
F
A
G
K
M
Fukugita et al (1996)
Brown et al. (2005)
11Our Search for more Hypervelocity Stars
O
B
F
A
G
K
M
Fukugita et al (1996)
Brown et al. (2006a)
12Our Search for more Hypervelocity Stars
O
B
F
A
G
K
M
Fukugita et al (1996)
Brown et al. (2006b)
13New Discoveries
Brown et al. (2006b)
astro-ph/0604111
14The Big Picture
Brown et al. (2006b)
-300 0
300 km/s
15Mass Function of Stars
We Observe 4 HVS in 4000 deg2
40 3-4 Msun HVSs
U. Heber
Salpeter
16 3-4 Msun stars
Predicted 2000 HVSs (Yu Tremaine)
Arches
460 3-4 Msun stars
NASA HST
16Applications Galactic
- Yu Tremaine (2003) HVS rates
- Gualandris et al (2005) velocities
- Ginsburg Loeb (2005) orbits
- Levin (2005) in-spiral signature
- Gnedin et al (2005) dark matter
Ginsburg Loeb (2006)
LISA
17Applications Extra-Galactic
M87
- Holley-Bockelmann et al. (2006)
- M87 planetary nebulae?
- Demarque Virani (2006)
- center of M31?
D. Malin
M31
J. Ware
Bender et al (2005)
18Coming Attractions
- Discovery surveys MMT, 1.5m.
- Spectroscopic identifications
- HET, VLT (Edelmann, Heber).
- Space velocities HST (Gnedin).
- Variability MDM (Stanek).
- N-body simulations (Bromley).
- Other unusual objects (Kewley).
19Conclusions
- MBH a hypervelocity stars.
- First HVS B star 709 km/s
- Now seven known HVSs.
- Provide constraints on mass function of stars
- and infall history of MBH.
NY Times
20The Hypervelocity Stars
Brown et al. (2006b)