Highly Ionized High-Velocity Clouds toward PKS 2155-304 and Markarian 509
Abstract
To gain insight into four highly ionized high-velocity clouds (HVCs) discovered by Sembach et al., we have analyzed data from the Hubble Space Telescope (HST) and Far Ultraviolet Spectroscopic Explorer (FUSE) for the PKS 2155-304 and Mrk 509 sight lines. We measure strong absorption in O VI and column densities of multiple ionization stages of silicon (Si II, III, and IV) and carbon (C II, III, and IV). We interpret this ionization pattern as a multiphase medium that contains both collisionally ionized and photoionized gas. Toward PKS 2155-304, for HVCs at -140 and -270 km s-1, respectively, we measure logN(OVI)=13.80+/-0.03 and logN(OVI)=13.56+/-0.06 from Lyman series absorption, we find logN(HI)=16.37+0.22-0.14 and 15.23+0.38-0.22. The presence of high-velocity O VI spread over a broad (100 km s-1) profile, together with large amounts of low-ionization species, is difficult to reconcile with the low densities, ne~5×10-6 cm-3, in the collisional/photoionization models of Nicastro et al., although the HVCs show a similar relation in N(Si IV)/N(C IV) versus N(C II)/N(C IV) to that of high-z intergalactic clouds. Our results suggest that the high-velocity O VI in these absorbers does not necessarily trace the warm-hot intergalactic medium but instead may trace HVCs with low total hydrogen column density. We propose that the broad high-velocity O VI absorption arises from shock ionization, at bow shock interfaces produced from infalling clumps of gas with velocity shear. The similar ratios of high ions for HVC Complex C and these highly ionized HVCs suggest a common production mechanism in the Galactic halo.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- April 2004
- DOI:
- 10.1086/382269
- arXiv:
- arXiv:astro-ph/0312105
- Bibcode:
- 2004ApJ...605..216C
- Keywords:
-
- Galaxy: Halo;
- ISM: Abundances;
- ISM: Clouds;
- Galaxies: Quasars: Absorption Lines;
- Ultraviolet: ISM;
- Astrophysics
- E-Print:
- 38 pages, including 10 figures. ApJ, 10 April, 2004. Replaced with accepted version