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23 April 2024
 
  » arxiv » astro-ph/0201351

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A FUSE Survey of Interstellar O VI Absorption in the Small Magellanic Cloud
Charles G. Hoopes ; Kenneth R. Sembach ; J. Christopher Howk ; Blair D. Savage ; Alex W. Fullerton ;
Date 21 Dec 2001
Subject astro-ph
AffiliationJHU), Kenneth R. Sembach (STScI), J. Christopher Howk (JHU), Blair D. Savage (Wisconsin), and Alex W. Fullerton (JHU
AbstractWe present the results of a FUSE survey of O VI 1031.93 Angstrom and 1037.62 Angstrom absorption toward 18 OB stars in the Small Magellanic Cloud (SMC). We detect O VI along every sight line. The average value of the O VI column density in the SMC is log =14.53. This value is 1.7 times higher than the average value for the Milky Way halo (perpendicular to the Galactic plane) of log N_perp(O VI)=14.29 found by FUSE, even though the SMC has much lower metallicity than the Galaxy. The column density in the SMC is higher along sight lines that lie close to star-forming regions, in particular NGC 346 in the northern part of the SMC. The standard deviation of the column densities for sight lines outside of NGC 346 is +/- 27%, somewhat lower than the deviation seen in the Milky Way halo. The lowest O VI column densities, log N(O VI)~14.3, occur in the central region and in the southeastern ``Wing’’ of the galaxy. Even these low column densities are as high as the Milky Way average, establishing the presence of a substantial, extended component of coronal gas in the SMC. The O VI absorption is always shifted to higher velocities than the main component of lower ionization gas. The O VI line widths are broader than expected for pure thermal broadening. We discuss several mechanisms that may be able to explain the observed properties of the hot gas, including supershells, a galactic fountain, and the infall of gas previously stripped from the SMC by tidal interactions with the Milky Way and the Large Magellanic Cloud. If a fountain produces the hot gas, the mass flux per unit surface area is ~0.02 M_sun/yr/kpc2.
Source arXiv, astro-ph/0201351
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