Related papers: Blue E/S0 galaxies: merger remnants or disk rebuil…
This paper is withdrawn because the results in the paper are included in a paper to be published in Mathematical and Computer Modelling.
We present HST/WFPC2 observations of the five bluest E+A galaxies (z~0.1) in the Zabludoff et al. sample to study whether their detailed morphologies are consistent with late-to-early type evolution and to determine what drives that…
This paper has been withdrawn.
This work presents high $S/N$ spectroscopic observations of a sample of six suspected merger remnants, selected primarily on the basis of H{\sc i} tidal debris detections. Single stellar population analysis of these galaxies indicates that…
This paper has been withdrawn.
This paper has been withdrawn due to upload of another version of it as a new preprint: gr-qc/0404097
This paper has been withdrawn due to submission of subsequent versions as a new preprint
This paper has been withdrawn since the material in these notes has been updated, and extended, in hep-th/0409031 and hep-th/0409033, and in work to follow.
This paper has been withdrawn. It will be split into two separate papers. New results will be added in both papers.
This paper has been withdrawn by the author. It will be replaced, substantially modified, by sections of the author's completed PhD thesis.
This paper has been withdrawn.
The paper is being withdrawn. A new submission will follow.
This paper is withdrawn.
This article has been removed. It has been superseded by gr-qc/0506097.
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Observations reveal a strong structural coupling between bulge and disc in S0 galaxies, which seems difficult to explain if they have formed from supposedly catastrophic events such as major mergers. We face this question by quantifying the…
This paper has been withdrawn due to a photometric calibration error.
This paper has been withdrawn.
We search for signatures of recent galaxy close interactions and mergers in a sample of 202 early-type galaxies in the local universe from the public SDSS Stripe82 deep images ($\mu_r \sim 28.5$ mag arcsec$^{-2}$). Using two different…
This paper has been withdrawn by the author due to some problems. Please contact me.