AAS 199th meeting, Washington, DC, January 2002
Session 65. FUSE Only
Display, Tuesday, January 8, 2002, 9:20am-6:30pm, Exhibit Hall
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[65.07] FUSE Observations of Degree-Scale Variations in Galactic Halo O VI
J.C. Howk (Johns Hopkins), B.D. Savage (Wisc), K.R. Sembach (STScI), C.G. Hoopes (Johns Hopkins)
We report Far Ultraviolet Spectroscopic Explorer (FUSE)
observations of interstellar O VI absorption in the halo of
the Milky Way towards 12 early-type stars in the Large
Magellanic Cloud (LMC) and 11 in the Small Magellanic Cloud
(SMC). The mean column densities of O VI associated with the
Galactic halo towards the LMC and SMC are log =
14.52(+0.10,-0.14) and 14.13(+0.14,-0.20), respectively,
where the uncertainties represent the standard deviations of
the individual measurements about the means. Significant
variations in the O VI column densities are observed over
all of the angular scales probed by our observations: 0.5 to
5.1 degrees towards the LMC and 0.05 to 3.3 degrees towards
the SMC. The maximum factors by which the O VI varies
between sight lines towards the LMC and SMC are
approximately 2.9 and 4.1, respectively. The column density
variations trace the structure of the hot ionized medium in
the Galactic halo on scales of <<80 to 800 pc towards the
LMC and <<5 to 400 pc towards the SMC (assuming the
absorption arises within the first 5 kpc above the Galactic
plane).
This work is based on data obtained for the Guaranteed Time
Team by the NASA-CNES-CSA FUSE mission. Financial support
has been provided by NASA contract NAS5-32985. JCH and KRS
recognize support from NASA Long Term Space Astrophysics
grant NAG5-3485.
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