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The Galactic Inner Halo: Searching for White Dwarfs and Measuring the Fundamental Galactic Constant, Vo/Ro | | Jasonjot S. Kalirai
; Harvey B. Richer
; Brad M. Hansen
; Peter B. Stetson
; Michael M. Shara
; Ivo Saviane
; R. Michael Rich
; Marco Limongi
; Rodrigo Ibata
; Brad K. Gibson
; Gregory G. Fahlman & James Brewer
; | | Date: |
1 Apr 2003 | | Journal: | Astrophys.J. 601 (2004) 277-288 | | Subject: | astro-ph | | Affiliation: | UBC), Harvey B. Richer (UBC), Brad M. Hansen (UCLA), Peter B. Stetson (HIA/NRC), Michael M. Shara (AMNH), Ivo Saviane (ESO), R. Michael Rich (UCLA), Marco Limongi (Oss. Roma), Rodrigo Ibata (Obs. Strasbourg), Brad K. Gibson (Swinburne Univ.), Gregory G | | Abstract: | We establish an extragalactic, zero-motion frame of reference within the deepest optical image of a globular star cluster, an HST 123-orbit exposure of M4 (GO 8679, cycle 9). The line of sight beyond M4 (l,b (deg) = 351,16) intersects the inner halo (spheroid) of our Galaxy at a tangent-point distance of 7.6 kpc (for Ro = 8 kpc). We isolate these spheroid stars from the cluster based on their proper motions over the 6-year baseline between these and previous epoch HST data (GO 5461, cycle 4). Distant background galaxies are also found on the same sight line using image-morphology techniques. This fixed reference frame allows us to independently determine the fundamental Galactic constant, Vo/Ro = 25.3 +/- 2.6 km/s/kpc, thus providing a velocity of the Local Standard of Rest, v = 202.7 +/- 24.7 km/s for Ro = 8.0 +/- 0.5 kpc. Secondly, the galaxies allow a direct measurement of M4’s absolute proper motion, mu_total = 22.57 +/- 0.76 mas/yr, in excellent agreement with recent studies. The clear separation of galaxies from stars in these deep data also allow us to search for inner-halo white dwarfs. We model the conventional Galactic contributions of white dwarfs along our line of sight and predict 7.9 (thin disk), 6.3 (thick disk) and 2.2 (spheroid) objects to the limiting magnitude at which we can clearly delineate stars from galaxies (V = 29). An additional 2.5 objects are expected from a 20% white dwarf dark halo consisting of 0.5 Mo objects, 70% of which are of the DA type. After considering the kinematics and morphology of the objects in our data set, we find the number of white dwarfs to be consistent with the predictions for each of the conventional populations. However, we do not find any evidence for dark halo white dwarfs. | | Source: | arXiv, astro-ph/0304036 | | Services: | Forum | Review | PDF | Favorites | |
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