ar X iv : a st ro - p h / 06 11 59 1 v 1 1 9 N ov 2 00 6 The Effect of Cluster Environment on Galaxy Evolution in the Pegasus I Cluster

نویسندگان

  • Jacqueline H. van Gorkom
  • Brian Chaboyer
چکیده

We present neutral hydrogen observations of 54 galaxies in the Pegasus cluster. The observations include single dish HI measurements, obtained with the Arecibo telescope for all 54 galaxies in the sample, as well as HI images, obtained with the VLA for 10 of these. The Arecibo profiles reveal an overall HI deficiency in the cluster, with ∼40% of the galaxies in the core of the cluster showing modest deficiencies of typically a factor of 2 – 3. The HI morphology of some galaxies shows that the HI disk is smaller than the optical disk and slightly offset from NASA/Jenkins Predoctoral Fellow.

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

ar X iv : a st ro - p h / 06 11 07 8 v 1 2 N ov 2 00 6 The sizes of galaxy halos in galaxy cluster Abell 1689

The multiple images observed in galaxy cluster Abell 1689 provide strong constraints not only on the mass distribution of the cluster but also on the ensemble properties of the cluster galaxies. Using parametric strong lensing models for the cluster, and by assuming well motivated scaling laws between the truncation radius s and the velocity dispersion σ of a cluster galaxy we are able to deriv...

متن کامل

ar X iv : a st ro - p h / 06 11 50 9 v 1 1 6 N ov 2 00 6 A Sr - Rich Star on the Main Sequence of Omega Centauri

Abundance ratios relative to iron for carbon, nitrogen, strontium and barium are presented for a metal-rich main sequence star ([Fe/H]=–0.74) in the globular cluster ω Centauri. This star, designated 2015448, shows depleted carbon and solar nitrogen, but more interestingly, shows an enhanced abundance ratio of strontium [Sr/Fe]≈1.6 dex, while the barium abundance ratio is [Ba/Fe]≤0.6 dex. At th...

متن کامل

ar X iv : a st ro - p h / 06 05 00 8 v 1 2 9 A pr 2 00 6 Simulations of globular clusters merging in galactic nuclear regions

We present the results of detailed N-body simulations regarding the interaction of four massive globular clusters in the central region of a triaxial galaxy. The systems undergo a full merging event, producing a sort of 'Super Star Cluster' (SSC) whose features are close to those of a superposition of the individual initial mergers. In contrast with other similar simulations, the resulting SSC ...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2006