Journal Article

Galaxies with background QSOs – I. A search for strong galactic Hα lines

Donald G. York, Lorrie A. Straka, Michael Bishof, Seth Kuttruff, David Bowen, Varsha P. Kulkarni, Mark Subbarao, Gordon Richards, Daniel Vanden Berk, Patrick B. Hall, Timothy Heckman, Pushpa Khare, Jean Quashnock, Lara Ghering and Sean Johnson

in Monthly Notices of the Royal Astronomical Society

Published on behalf of The Royal Astronomical Society

Volume 423, issue 4, pages 3692-3708
Published in print July 2012 | ISSN: 0035-8711
Published online July 2012 | e-ISSN: 1365-2966 | DOI: http://dx.doi.org/10.1111/j.1365-2966.2012.21166.x
Galaxies with background QSOs – I. A search for strong galactic Hα lines

More Like This

Show all results sharing this subject:

  • Astronomy and Astrophysics

GO

Show Summary Details

Preview

A search for emission lines in foreground galaxies in quasar spectra (zgal < zQSO) of the Sloan Digital Sky Survey data release 5 reveals 23 examples of quasars shining through low redshift, foreground galaxies at small impact parameters (<10 kpc). About 74 000 quasar spectra were examined by searching for narrow Hα emission lines at z < 0.38, at a flux level greater than 5 × 10−17 erg cm−2 s−1, and then confirming that other expected emission lines of the H ii regions in the galaxy are detected. The galaxies were deblended from the quasar images to get colours and morphologies. For cases that allow the galaxy and the quasar to be deblended, the galaxies are blue (0.95 < (ur) < 1.95). Extinction and reddening through the galaxies are determined from the (gi) colour excess of the quasars. These reddening values are compared with the flux ratio of Hα to Hβ, which reflect the extinction for an undetermined fraction of the sightline through each galaxy. No trends were found relating E(BV)(gi), impact parameter (b), and (ur) for the galaxies or between E(BV) derived from (gi) and that derived from Hα/Hβ. Comparison with previous studies of quasar absorption systems indicates that our sample is more reddened, suggesting disc-dominated absorber galaxies. Measurement or limits on galactic, interstellar Ca ii and Na i absorption lines are given from the quasar spectrum. No trends were found relating the Ca ii equivalent width W (Ca ii) or the Na i equivalent width W (Na i) to b, but a correlation of rs=−0.77 (α= 0.05) was found relating W (Ca ii) and E(BV)(gi).

Keywords: galaxies: evolution; galaxies: photometry; quasars: absorption lines; cosmology: observations

Journal Article.  8038 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.