Journal Article

On the sizes of neutral hydrogen regions giving rise to damped Lyα absorption systems*

E. M. Monier, D. A. Turnshek and S. Rao

in Monthly Notices of the Royal Astronomical Society

Published on behalf of The Royal Astronomical Society

Volume 397, issue 2, pages 943-953
Published in print August 2009 | ISSN: 0035-8711
Published online July 2009 | e-ISSN: 1365-2966 | DOI: http://dx.doi.org/10.1111/j.1365-2966.2009.15000.x
On the sizes of neutral hydrogen regions giving rise to damped Lyα absorption systems*

More Like This

Show all results sharing this subject:

  • Astronomy and Astrophysics

GO

Show Summary Details

Preview

Using quasi-stellar object (QSO) absorption-line spectra obtained along closely spaced sightlines, we examine the transverse sizes of regions containing large columns of neutral hydrogen gas at redshifts z≈ 1.5. The observations are primarily of intervening damped Lyα (DLA) and sub-DLA absorption-line systems in gravitationally lensed QSOs. In particular, Hubble Space Telescope spectroscopy of the four-component Cloverleaf QSO (H1413+1143) reveals three new DLA/sub-DLA systems at z≈ 1.44, 1.49 and 1.66. A neutral hydrogen column density of NH i≥ 2 × 1020 atoms cm−2 is required for a system to be classified as a DLA, but none of the three systems has an H i column density above the DLA threshold in all four components. Over component separations <1.4 arcsec in the Cloverleaf, corresponding to transverse sizes of ≈5–12 h−170 kpc, the H i column densities typically change by factors of ≈2–40. Similar observations of other QSOs containing absorption systems in the DLA regime are summarized from the literature. In addition to establishing approximate sizes for DLA regions, the results have implications for their volume-averaged H i gas number densities and neutral gas masses. By combining our results on DLA absorber sizes with published results on the sizes of lower column density QSO absorbers, which however arise in very ionized regions, we infer the useful relation that the typical transverse size of an absorber in the redshift interval z≈[1, 2] is Sabs≈ 11 h−170[NH i/1020]−1/4 kpc.

Keywords: intergalactic medium; quasars: absorption lines; quasars: individual: H1413+1143

Journal Article.  8820 words.  Illustrated.

Subjects: Astronomy and Astrophysics

Full text: subscription required

How to subscribe Recommend to my Librarian

Users without a subscription are not able to see the full content. Please, subscribe or login to access all content.