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19992001
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astro-ph2001

Disk Contamination in a sample of proper motion selected halo stars: A Comment on "Direct Detection of Galactic Halo Dark Matter", B.A. Oppenheimer et al., Science

David S. Graff

Based on a proper motion survey, Oppenheimer et al. claim the detection of a white dwarf component of the dark matter of the halo. I show that most of the white dwarfs in their sam…

astro-ph2001

Using the Supernova / Acceleration Probe (SNAP) to Search for Microlensing Events Towards the LMC

David S. Graff, Alex Kim

Microlensing experiments today have a tantalizing result; they have detected an excess of microlensing events beyond what is expected from known stellar populations. These events c…

astro-ph2000

Death of Stellar Baryonic Dark Matter Candidates

Katherine Freese, Brian Fields, David Graff

The nature of the dark matter in the Universe is one of the outstanding questions in astrophysics. In this talk, I address possible stellar baryonic contributions to the 50-90% of…

astro-ph2000

What are MACHOs? Interpreting LMC microlensing

David S. Graff

I discuss two hypotheses that might explain LMC microlensing: the Halo stellar remnant lensing hypothesis and the unvirialized LMC lensing hypothesis. I show that white dwarfs cann…

astro-ph2000

High Velocity Star Formation in the LMC

David S. Graff, Andrew P. Gould

Light-echo measurements show that SN1987A is 425 pc behind the LMC disk. It is continuing to move away from the disk at $18 \kms$. Thus, it has been suggested that SN1987A was ejec…

astro-ph1999

The velocity dispersion of LMC Carbon stars: possible detection of a kinematically distinct population

David S. Graff, Andrew P. Gould, Nicholas Suntzeff +2

We analyze the velocity residuals of 551 carbon stars relative to a rotating-disk model of the inner of the Large Magellanic Cloud (LMC). We find that the great…