Journal Article

Spatially resolved medium resolution spectroscopy of an interacting E+A (post-starburst) system with the Subaru Telescope*

Tomotsugu Goto, Masafumi Yagi and Chisato Yamauchi

in Monthly Notices of the Royal Astronomical Society

Published on behalf of The Royal Astronomical Society

Volume 391, issue 2, pages 700-710
Published in print December 2008 | ISSN: 0035-8711
Published online November 2008 | e-ISSN: 1365-2966 | DOI: https://dx.doi.org/10.1111/j.1365-2966.2008.13891.x
Spatially resolved medium resolution spectroscopy of an interacting E+A (post-starburst) system with the Subaru Telescope*

More Like This

Show all results sharing this subject:

  • Astronomy and Astrophysics

GO

Show Summary Details

Preview

We have performed spatially resolved medium resolution long-slit spectroscopy of a nearby E+A (post-starburst) galaxy system, SDSS J161330.18+510335.5, with the FOCAS spectrograph mounted on the Subaru Telescope. This E+A galaxy has an obvious companion galaxy 14 kpc in front with the velocity difference of 61.8 km s−1. Both galaxies have obviously disturbed morphology. Thus, this E+A system provides us with a perfect opportunity to investigate the relation between the post-starburst phenomena and galaxy–galaxy interaction.

We have found that the Hδ equivalent width (EW) of the E+A galaxy is greater than 7 Å galaxy wide (8.5 kpc) with no significant spatial variation. The E+A galaxy has a weak [O iii] emission (EW ∼ 1 Å) offset by ∼2.6 kpc from the peak of the Balmer absorption lines. We detected a rotational velocity in the companion galaxy of >175 km s−1. The progenitor of the companion may have been a rotationally supported, but yet passive S0 galaxy. We did not detect significant rotation on the E+A galaxy. A metallicity estimate based on the rH colour suggests Z= 0.008 and 0.02, for the E+A and the companion galaxies, respectively. Assuming these metallicity estimates, the age of the E+A galaxy after quenching the star formation is estimated to be 100–500 Myr, with its centre having a slightly younger stellar population. The companion galaxy is estimated to have an older stellar population of >2 Gyr of age with no significant spatial variation.

These findings are inconsistent with a simple picture where the dynamical interaction creates infall of the gas reservoir that causes the central starburst/post-starburst. Instead, our results present an important example where the galaxy–galaxy interaction can trigger a galaxy-wide post-starburst phenomenon.

Keywords: galaxies: evolution; galaxies: formation; galaxies: interactions; galaxies: peculiar; galaxies: starburst

Journal Article.  7482 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.