Central Stellar Populations of S0 Galaxies in The Fornax Cluster

Based on FORS2-VLT long-slit spectroscopy, the analysis of the central absorption line indices of 9 S0 galaxies in the Fornax Cluster is presented. Central indices correlate with central velocity dispersions as observed in ellipticals. However, the stellar population properties of these S0s indicates that the observed trends are produced by relative differences in age and alpha-element abundances and not in metallicity ([Fe/H]) as previous studies have found in elliptical galaxies. The observed scatter in the line indices vs. velocity dispersion relations can be partially explained by the rotationally-supported nature of many of these systems. The presence of tighter line indices vs. maximum (circular) rotational velocity relations confirms this statement. It was also confirmed that the dynamical mass is the driving physical property of all these correlations and in our Fornax S0s it has to be estimated assuming rotational support.Comment: To appear in the Proceedings of IAU Symposium 241: "Stellar Populations as Building Blocks of Galaxies", 10-16 December, 2006 at La Palma, Canary Islands, Spai

Four new species of Acalypha L. (Euphorbiaceae, Acalyphoideae) from Madagascar, with notes about their conservation status

Marisa, dejo sin poner identificadores de proyecto porque en CORDIS no he logrado encontrar dos de los que se trata en el Funding. Faltan dígitos, la información que aporta creo que es incompleta. Llevo mucho tiempo buscando y no encuentro nada.Yo, Estrella, tampoco he encontrado esos identificadores en Cordis y también los he buscado por el nombre de proyecto que aparece en el fundingFour new species of Acalypha, subgen. Acalypha (Euphorbiaceae, Acalyphoideae) from Madagascar are described, illustrated, and mapped. Acalypha ankaranensis sp. nov. is found in the Anakarana massif, in a dry deciduous forest at 180 m elevation; A. cardielii sp. nov. in the Tsingy de Bemaraha, also associate to dry deciduous forest, at 360 m elevation; A. magistri sp. nov. in the Marojejy Natural Reserve, in evergreen moist forest at 1583 m elevation, and A. levinii sp. nov. in the southern sclerophyllous woodland between 140 to 990 m elevation. These new species are quite well characterized morphologically and ecologically and are easily differentiated from morphologically similar ones. A. ankaranensis and A. levinii are most similar to A. paxii Aug.DC., a common species in northern Magdagascar, A. cardielii is close to A. leptomyura Baill, and A. magistri is close to A. chibomboa Baill. According to our preliminary conservation assessments, A. ankaranensis and A. cardielii are Critically Endangered, A. levinii is Endangered, and A. magistri is VulnerableThis research has received support from the SYNTHESYS Project (http://www.synthesys.info/; FR-TAF 6307) financed by European Community Research Infrastructure Action under the FP7 "Capaci ties" Program; also from the European Molecular Biology Organiza tion (https://www.embo.org; STF-8222). We kindly thank the curators and staff of the herbaria mentioned for facilitating the study of their specimens, and Laura Gonzalez Hern andez, author of the excellent illustrations included in this work. Finally, our gratitude to Louis Nusbaumer, and the anonymous reviewers, that have helped us to improve the submitted manuscrip

Four new species of Acalypha L. (Euphorbiaceae, Acalyphoideae) from the West Indian Ocean Region

Four new species of Acalypha (Euphorbiaceae, Acalyphoideae) from the Western Indian Ocean Region, based on morphological and molecular evidence, are described, illustrated, and mapped. Acalypha gillespieae sp. nov., A. leandrii sp. nov. and A. nusbaumeri sp. nov. are endemic to Madagascar, and A. mayottensis sp. nov. is known only from Mbouzi islet (Mayotte), in the Comoros Archipelago. We also describe for the first time in Acalypha the presence of membranous or chartaceous perules covering the axillary buds. Preliminary conservation assessments of the new species are also providedThis research received support from the SYNTHESYS Project (http://www.synthesys. info/; FR-TAF 6307, DE-TAF 3319, and SE-TAF 5590) financed by European Community Research Infrastructure Action under the FP7 “Capacities” Program, the European Molecular Biology Organization (https://www.embo.org; STF-8222), and the United States National Science Foundation (DEB-0128872

Evolution of the anti-truncated stellar profiles of S0 galaxies since z=0.6z=0.6 in the SHARDS survey: I - Sample and Methods

The controversy about the origin of the structure of S0--E/S0 galaxies may be due to the difficulty of comparing surface brightness profiles with different depths, photometric corrections and PSF effects (almost always ignored). We aim to quantify the properties of Type-III (anti-truncated) discs in a sample of S0 galaxies at 0.2<z<0.6. In this paper, we present the sample selection and describe in detail the methods to robustly trace the structure in their outskirts and correct for PSF effects. We have selected and classified a sample of 150 quiescent galaxies at 0.2<z<0.6 in the GOODS-N field. We perform a quantitative structural analysis of 44 S0-E/S0 galaxies. We corrected their surface brightness profiles for PSF distortions and analysed the biases in the structural and photometric parameters when the PSF correction is not applied. Additionally, we have developed Elbow, an automatic statistical method to determine whether a possible break is significant - or not - and its type and made it publicly available. We found 14 anti-truncated S0-E/S0 galaxies in the range 0.2<z<0.6 (~30% of the final sample). This fraction is similar to the those reported in the local Universe. In our sample, ~25% of the Type-III breaks observed in PSF-uncorrected profiles are artifacts, and their profiles turn into a Type I after PSF correction. PSF effects also soften Type-II profiles. We found that the profiles of Type-I S0 and E/S0 galaxies of our sample are compatible with the inner profiles of the Type-III, in contrast with the outer profiles. We have obtained the first robust and reliable sample of 14 anti-truncated S0--E/S0 galaxies beyond the local Universe, in the range 0.2<z<0.6. PSF effects significantly affect the shape of the surface brightness profiles in galaxy discs even in the case of the narrow PSF of HST/ACS images, so future studies on the subject should make an effort to correct them.Comment: Accepted for publishing in Astronomy & Astrophysics. 75 pages, 57 figure

Adapting the revised prenatal coping inventory (NuPCI) for use in a Spanish population

Objective: To adapt the Revised Prenatal Coping Inventory (NuPCI) for the evaluation of prenatal stress coping strategies utilised by Spanish women. Methods: A cross-sectional study was performed to evaluate the psychometric properties of NuPCI adapted for a Spanish population. Two hundred and sixty one puerperium women completed the NuPCI at the time of discharge after childbirth. Instrument construct validity was evaluated using subscale item correlations. Internal consistency was assessed using Cronbach’s a test. Results: Items from each subscale (Preparation, Avoidance and Spiritual – Positive Coping) were significantly correlated with the global result (p¿¿0.7). The most frequently used coping strategy was Preparation and the least used was Avoidance. Utilisation of the coping strategies with Preparation decreased with increasing parity (p¿=¿.002) and greater prenatal stress was associated with increased use of the Avoidance coping strategy (p¿<¿.001). Conclusions: The NuPCI adapted for Spanish women demonstrates good psychometric properties for evaluating the three types of prenatal stress coping strategies: Preparation, Avoidance and Spiritual – Positive Coping. Results were similar to those presented by the instrument in its English language version

Morphologies and stellar populations of galaxies in the core of Abell 2218

SUMMARIZED ABSTRACT: We present a study of the stellar populations and morphologies of galaxies in the core of the galaxy cluster Abell 2218. Integral field spectroscopy was obtained using PMAS/[email protected] CAHA to obtain a complete flux limited sample of cluster members within its field-of-view (~74"X64"). In addition of 31 galaxies with known redshifts in the outer regions, we built up a final sample of 59 spectroscopically confirmed cluster members. Multiban photometry and detailed morphologies were obtained using deep images taken with the HST/ACS camera in the BVRI and z-bands. The CM diagram shows that the E-type galaxies cover the range of brighter and redder colors. A large fraction of spiral galaxies ($\sim$50%) is found. They cover a wide range in colors. This result, together with the distributions of ages, metallicities and masses, indicates that E-type galaxies are more massive and have older stellar populations, while L-type galaxies are less massive and have a wider range of stellar Our results agree with a proposed two-step scenario for the evolution of galaxies in clusters. In addition, an extremely blue merging galaxy system is found at the core, with the nominal redshift of the cluster.Comment: 29 pages, 17 figures, accepted for publishing in MNRAS. (HST/ACS composite image: http://www.caha.es/sanchez/abell2218/BRI_big.jpg