Related papers: Blue E/S0 galaxies: merger remnants or disk rebuil…
This paper has been withdrawn because the models on which it was based have undergone significant changes and improvements. A new paper with the same title, based on the improved models, is accepted for publication in MNRAS and is available…
Studying outliers from the bimodal distribution of galaxies in the color-mass space, such as morphological early-type galaxies residing in the blue cloud, can help to better understand the physical mechanisms that lead galaxy migrations in…
This paper has been withdrawn by the author(s), since it has been merged with paper I (astro-ph/0307482).
This paper has been withdrawn.
This paper has been withdrawn. The contents of this paper can now be found in 0907.3000, which combines the erstwhile 0901.2981 and 0901.2982 in a somewhat compact form.
The paper has been withdrawm. A completely new version on oscillating axionic boson stars will appear.
This paper has been withdrawn by the author. It will be posted on astro-ph once the proceedings of the 363rd Heraeus Seminar on Neutron Stars and Pulsars are ready.
This paper has been withdrawn by the author, because a better treatment is given in the author's Phd. thesis (Sections 3.4.6 and 4.4), now available on the arxiv.
A modified version of this paper is under process and with a new title and abstract. Hence, this version of the article is completely withdrawn.
This paper has been withdrawn by the author because has been send to other journal.
The paper has been withdrawn
This paper has been withdrawn.
We identify a population of morphologically defined E/S0 galaxies lying on the blue sequence at the present epoch. Using three samples, we analyze blue-sequence E/S0s with stellar masses >10^8 Msun, arguing that individual objects may be…
This paper has been withdrawn. A significantly revised version will be posted in the near future.
This paper has been withdrawn by the authors due to the existence of main results in the literature.
This paper has been withdrawn. The contents of this paper can now be found in 0907.3000, which combines the erstwhile 0901.2981 and 0901.2982 in a somewhat compact form.
This paper has been withdrawn: it has been merged with the preprint to which it refers.
We examine the HI+H_2 content of blue-sequence E/S0s -- a recently identified population of galaxies that are morphologically early type, but reside alongside spiral galaxies in color vs. stellar mass space. We test the idea that the…
This paper has been withdrawn
This paper is withdrawn. The revised paper appears in chao-dyn/9904020