Evidence of coupling between the thermal and nonthermal emission in the gamma-ray binary LS I +61 303

The gamma-ray binary LS I +61 303 is composed of a Be star and a compact companion orbiting in an eccentric orbit. Variable flux modulated with the orbital period of ~26.5 d has been detected from radio to very high-energy gamma rays. In addition, the system presents a superorbital variability of the phase and amplitude of the radio outburst with a period of ~4.6 yr. We present optical photometric observations of LS I +61 303 spanning ~1.5 yr and contemporaneous Halpha equivalent width (EW Halpha) data. The optical photometry shows, for the first time, that the known orbital modulation suffers a positive orbital phase shift and an increase in flux for data obtained 1-yr apart. This behavior is similar to that already known at radio wavelengths, indicating that the optical flux follows the superorbital variability as well. The orbital modulation of the EW Halpha presents the already known superorbital flux variability but shows, also for the first time, a positive orbital phase shift. In addition, the optical photometry exhibits a lag of ~0.1-0.2 in orbital phase with respect to the EW Halpha measurements at similar superorbital phases, and presents a lag of ~0.1 and ~0.3 orbital phases with respect noncontemperaneous radio and X-ray outbursts, respectively. The phase shifts detected in the orbital modulation of thermal indicators, such as the optical flux and the EW Halpha, are in line with the observed behavior for nonthermal indicators, such as X-ray or radio emission. This shows that there is a strong coupling between the thermal and nonthermal emission processes in the gamma-ray binary LS I +61 303. The orbital phase lag between the optical flux and the EW Halpha is naturally explained considering different emitting regions in the circumstellar disk, whereas the secular evolution might be caused by the presence of a moving one-armed spiral density wave in the disk.Comment: 4 pages, 3 figures, accepted for publication in A&A (this version matches the published version

Aplicación de la genética en la identificación de enfermedades infecciosas bucodentales

La genética ha supuesto una gran revolución en la identificación de seres vivos a través de análisis de ADN. Actualmente se investiga la pos1bilidad de aplicarla en el estudio de nuestros antepasados, desde el hombre prehistórico. En el ámbito de la odontologfa se vislumbran nuevas perspectivas en el estudio de la patologfa infecciosa, gracias a estos avances en biologfia molecular. El presente trabajo pretende repasar cuál ha sido esta patología infecciosa en el hombre del pasado y cuáles son Jos métodos de análisis genético que penniten estudiarla. Fundamentalmente, las infecciones bucodentales del hombre prehistórico se resumen en caries y patología periodontal. La RCP (reacción en cadena de la polimerasa) es la técnica que ha revolucionado la ingeniería genética, pues permite obtener copias del ADN para poder ser analizado y, con ello, ofrece un diagnóstico específico de la etiología de las enfermedades infecciosas, lográndose una identificación más precisa que con el cultivo o con la inmunohistoquímica de las bacterias, hongos y virus que conviven en el medio oral

The Alignment between Satellites and Central Galaxies: Theory vs. Observations

Recent studies have shown that the distribution of satellite galaxies is preferentially aligned with the major axis of their central galaxy. The strength of this alignment has been found to depend strongly on the colours of the satellite and central galaxies, and only weakly on the mass of the halo in which the galaxies reside. In this paper we study whether these alignment signals, and their dependence on galaxy and halo properties, can be reproduced in a hierarchical structure formation model of a $\Lambda$CDM concordance cosmology. To that extent we use a large $N$-body simulation which we populate with galaxies following a semi-analytical model for galaxy formation. We find that if the orientation of the central galaxy is perfectly aligned with that of its dark matter halo, then the predicted central-satellite alignment signal is much stronger than observed. If, however, the minor axis of a central galaxy is perfectly aligned with the angular momentum vector of its dark matter halo, we can accurately reproduce the observed alignment strength as function of halo mass and galaxy color. Although this suggests that the orientation of central galaxies is governed by the angular momentum of their dark matter haloes, we emphasize that any other scenario in which the minor axes of central galaxy and halo are misaligned by $\sim 40^{\circ}$ (on average) will match the data equally well. Finally, we show that dependence of the alignment strength on the color of the central galaxy is most likely an artefact due to interlopers in the group catalogue. The dependence on the color of the satellite galaxies, on the other hand, is real and owes to the fact that red satellites are associated with subhaloes that were more massive at their time of accretion.Comment: 13 Pages, 10 Figures, one figure replaced. added in discussion about comparison with others results, Updated version to match accepted version to MNRA

Properties of Galaxy Groups in the SDSS: II.- AGN Feedback and Star Formation Truncation

Successfully reproducing the galaxy luminosity function and the bimodality in the galaxy distribution requires a mechanism that can truncate star formation in massive haloes. Current models of galaxy formation consider two such truncation mechanisms: strangulation, which acts on satellite galaxies, and AGN feedback, which predominantly affects central galaxies. The efficiencies of these processes set the blue fraction of galaxies as function of galaxy luminosity and halo mass. In this paper we use a galaxy group catalogue extracted from the Sloan Digital Sky Survey (SDSS) to determine these fractions. To demonstrate the potential power of this data as a benchmark for galaxy formation models, we compare the results to the semi-analytical model for galaxy formation of Croton et al. (2006). Although this model accurately fits the global statistics of the galaxy population, as well as the shape of the conditional luminosity function, there are significant discrepancies when the blue fraction of galaxies as a function of mass and luminosity is compared between the observations and the model. In particular, the model predicts (i) too many faint satellite galaxies in massive haloes, (ii) a blue fraction of satellites that is much too low, and (iii) a blue fraction of centrals that is too high and with an inverted luminosity dependence. In the same order, we argue that these discrepancies owe to (i) the neglect of tidal stripping in the semi-analytical model, (ii) the oversimplified treatment of strangulation, and (iii) improper modeling of dust extinction and/or AGN feedback. The data presented here will prove useful to test and calibrate future models of galaxy formation and in particular to discriminate between various models for AGN feedback and other star formation truncation mechanisms.Comment: 16 pages, 5 figures, submitted to MNRA

L’impacte de la cabra (Capra hircus) sobre el teix (Taxus baccata) a l’illa de Mallorca

[cat] El teix Taxus baccata a les Balears es troba únicament a la Serra de Tramuntana, està protegit com d’Especial Protecció i és objecte d’un Pla de Maneig executat per la Conselleria de Medi Ambient del Govern de les Illes Balears. La forta pressió de les cabres Capra hircus, incrementada els darrer decennis per l’abandonament de les finques i l’agricultura, és una amenaça que fa perillar el futur del teix. El present treball completa i revisa l’inventari de teixos naturals a la Serra i avalua el seu estat de conservació en funció del grau d’afectació per les cabres assilvestrades. Un 70% dels teixos silvestres pateixen impactes visibles provocats per les cabres. Tot i que la majoria de teixos es trobem empenyalats, la gran majoria (un 84%) pateix un grau d’afectació moderat; el 14% restant presenta una afectació greu, amb una clara amenaça per a la seva supervivència. Els teixos menys afectats són els més difícilment accessibles, i no hi ha cap opció de que puguin créixer amb normalitat a un lloc on arribin les cabres. Ara que ja no es talla ni es permeten les cremes descontrolades, el teix podria tenir unes poblacions més nombroses, tot i que les elevades temperatures estivals i la disminució de les precipitacions, com a conseqüència del canvi climàtic, podrien esdevenir un factor limitant. Avui, però, el principal factor limitant no natural que afecta les poblacions de teix a Mallorca és la pressió que exerceixen les cabres assilvestrades les quals, en molts de casos, poden arribar a provocar la mort dels exemplars.[eng] The yew Taxus baccata in the Balearic Islands is only in the Serra de Tramuntana. It is under Special Protection category and is object of a Management Plan executed by the Balearic Environmental Administration. The strong pressure of goats Capra hircus, increased over the last decades due to the abandonment of farms and agriculture, is a threat that endangers yews future. The present report completes and reviews the inventory of natural yews in the Serra and evaluates its state of conservation based on the degree of involvement by the wild goats. 70% of natural yews suffer visible impacts caused by goats. Although most yews are in cliffs, the vast majority (84%) suffers a moderate degree of threat; the remaining 14% have a serious affectation, with a clear threat to their survival. The least-affected yews are the most difficult to reach, and there is no option to grow normally on a goat's place. Now that neither the cutting of yew or the uncontrolled burning are not allowed, the yew tree could have larger populations, although the high summer temperatures and the decrease of the precipitations, as a consequence of the climate change, could become a limiting factor. Today, however, the main unnatural limiting factor affecting yew populations in Mallorca is the pressure exerted by feral goats which, in many cases, may cause the death of specimens