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Theory of pixel lensing towards M31 -- II. The velocity anisotropy and flattening of the MACHO distribution | | The POINT--AGAPE Collaboration: E. Kerins
; J. An
; N.W. Evans
; P. Baillon
; B.J. Carr
; Y. Giraud-Heraud
; A. Gould
; P. Hewett
; J. Kaplan
; S. Paulin-Henriksson
; S.J. Smartt
; Y. Tsapras
; D. Valls-Gabaud
; | | Date: |
15 Jul 2003 | | Journal: | Astrophys.J. 598 (2003) 993-999 DOI: 10.1086/379060 | | Subject: | astro-ph | | Affiliation: | Liverpool JMU), J. An (Cambridge), N.W. Evans (Cambridge), P. Baillon (CERN), B.J. Carr (Queen Mary, London), Y. Giraud-Heraud (College de France), A. Gould (Ohio State), P. Hewett (Cambridge), J. Kaplan (College de France), S. Paulin-Henriksson (Coll | | Abstract: | The POINT-AGAPE collaboration is currently searching for massive compact halo objects (MACHOs) towards the Andromeda galaxy (M31). The survey aims to exploit the high inclination of the M31 disk, which causes an asymmetry in the spatial distribution of M31 MACHOs. Here, we investigate the effects of halo velocity anisotropy and flattening on the asymmetry signal using simple halo models. For a spherically symmetric and isotropic halo, we find that the underlying pixel-lensing rate in far-disk M31 MACHOs is more than 5 times the rate of near-disk events. We find that the asymmetry is increased further by about 30% if the MACHOs occupy radial orbits rather than tangential orbits, but is substantially reduced if the MACHOs lie in a flattened halo. However, even for haloes with a minor-to-major axis ratio q = 0.3, the numbers of M31 MACHOs in the far-side outnumber those in the near-side by a factor of ~2. We show that, if positional information is exploited in addition to number counts, then the number of candidate events required to confirm asymmetry for a range of flattened and anisotropic halo models is achievable, even with significant contamination by variable stars and foreground microlensing events. For pixel-lensing surveys which probe a representative portion of the M31 disk, a sample of around 50 candidates is likely to be sufficient to detect asymmetry within spherical haloes, even if half the sample is contaminated, or to detect asymmetry in haloes as flat as q = 0.3 provided less than a third of the sample comprises contaminants. We also argue that, provided its mass-to-light ratio is less than 100, the recently observed stellar stream around M31 is not problematic for the detection of asymmetry. (Abstract slightly abridged.) | | Source: | arXiv, astro-ph/0307284 | | Services: | Forum | Review | PDF | Favorites | |
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