Warm gas in the rotating disk of the Red Rectangle: accurate models of molecular line emission

We aim to study the excitation conditions of the molecular gas in the rotating disk of the Red Rectangle, the only post-Asymptotic-Giant-Branch object in which the existence of an equatorial rotating disk has been demonstrated. For this purpose, we developed a complex numerical code that accurately treats radiative transfer in 2-D, adapted to the study of molecular lines from rotating disks. We present far-infrared Herschel/HIFI observations of the 12CO and 13CO J=6-5, J=10-9, and J=16-15 transitions in the Red Rectangle. We also present our code in detail and discuss the accuracy of its predictions, from comparison with well-tested codes. Theoretical line profiles are compared with the empirical data to deduce the physical conditions in the disk by means of model fitting. We conclude that our code is very efficient and produces reliable results. The comparison of the theoretical predictions with our observations reveals that the temperature of the Red Rectangle disk is typically ~ 100-150 K, about twice as high as previously deduced from mm-wave observations of lower-J lines. We discuss the relevance of these new temperature estimates for understanding the thermodynamics and dynamics of this prototype object, as well as for interpreting observations of other rarely studied post-AGB disks. Despite our sophisticated treatment of the line formation, our model cannot explain the relatively strong line-wing emission for intermediate-J transitions. We argue that a model including a rotating disk only cannot reproduce these data and suggest that there is an additional extended (probably bipolar) structure expanding at about 7--15 km/s.Comment: 18 pages, 21 figure

The molecular envelope of CRL 618: A new model based on Herschel/HIFI observations

We study the physical properties and molecular excitation of the different warm gas components found in the protoplanetary nebula CRL 618. We revise our previous Herschel/HIFI observations, which consist of several 12CO and 13CO lines in the far-infrared/sub-mm band. These data have been re-analyzed in detail by improving calibration, the signal-to-noise-ratio, and baseline substraction. We identify the contributions of the different nebular components to the line profiles. We have used a spatio-kinematical model to better constrain the temperature, density, and kinematics of the molecular components probed by the improved CO observations. The 12CO and 13CO J=16-15, J=10-9, and J=6-5 transitions are detected in this source. The line profiles present a composite structure showing spectacular wings in some cases, which become dominant as the energy level increases. Our analysis of the high-energy CO emission with the already known low-energy J=2-1 and J=1-0 lines confirms that the high-velocity component, or fast bipolar outflow, is hotter than previously estimated with a typical temperature of ~300 K. This component may then be an example of a very recent acceleration of the gas by shocks that has not yet cooled down. We also find that the dense central core is characterized by a very low expansion velocity, ~5 km/s, and a strong velocity gradient. We conclude that this component is very likely to be the unaltered circumstellar layers that are lost in the last AGB phase, where the ejection velocity is particularly low. The physical properties of the other two nebular components, the diffuse halo and the double empty shell, more or less agrees with the estimations derived in previous models.Comment: Accepted for publication in Astronomy & Astrophysics. 8 pages, 3 figure

Detection of Keplerian dynamics in a disk around the post-AGB star AC Her

So far, only one rotating disk has been clearly identified and studied in AGB or post-AGB objects (in the Red Rectangle), by means of observations with high spectral and spatial resolution. However, disks are thought to play a key role in the late stellar evolution and are suspected to surround many evolved stars. We aim to extend our knowledge on these structures. We present interferometric observations of CO J=2-1 emission from the nebula surrounding the post-AGB star AC Her, a source belonging to a class of objects that share properties with the Red Rectangle and show hints of Keplerian disks. We clearly detect the Keplerian dynamics of a second disk orbiting an evolved star. Its main properties (size, temperature, central mass) are derived from direct interpretation of the data and model fitting. With this we confirm that there are disks orbiting the stars of this relatively wide class of post-AGB objectsComment: 4 pages, 3 figure

The radio continuum spectrum of Mira A and Mira B up to submillimeter wavelengths

We present new measurements of the flux densities at submillimeter wavelengths based on ALMA band 7 (338 GHz) and band 9 (679 GHz) observations to better constrain the origin of the continuum emission of the Mira AB binary system and to check its orbit. We have measured the Mira A and Mira B continuum in ALMA band 7, with a resolution of ~0"31, and for the first time in ALMA band 9, with a resolution of ~0"18. We resolved the binary system at both bands, and derived the continuum spectral index of the stars and their relative position. We also analyzed ALMA SciVer data obtained in bands 6 and 3. Measurements at centimeter wavelengths obtained by other authors have been included in our study of the spectral energy distribution of the Mira components. The Mira A continuum emission has a spectral index of 1.98+-0.04 extending from submillimeter down to centimeter wavelengths. The spectral index of the Mira B continuum emission is 1.93+-0.06 at wavelengths ranging from submillimeter to ~3.1 mm, and a shallower spectral index of 1.22+-0.09 at longer wavelengths. The Mira A continuum emission up to submillimeter wavelengths is consistent with that of a radio photosphere surrounding the evolved star for which models predict a spectral index close to 2. The Mira B continuum emission cannot be described with a single ionized component. An extremely compact and dense region around the star can produce the nearly thermal continuum measured in the 0.4-3.1 mm wavelength range, and an inhomogeneous, less dense, and slightly larger ionized envelope could be responsible for the emission at longer wavelengths. Our results illustrate the potential of ALMA for high precision astrometry of binary systems. We have found a significant discrepancy of ~14 milliarcsec between the ALMA measurements and the predicted orbit positions.Comment: 6 pages, 3 figures, 2 tables, accepted for publication in Astronomy and Astrophysic

Josep Lluís Blasco Estellés (1940-2003)

Josep Lluís Blasco Estellés (Sagunt 1940 – Valencia 2003) was one of the prominent introducers of analytic philosophy into the Catalan Countries in the 20th century. Initially an adherent of ordinary language philosophy within analytic philosophy, he later became an acute commentator of Quine, Wittgenstein, Kant and logical positivism

Roles de género y jóvenes: la imagen televisiva que vende

belleza, delgadez, sumisión, eterna juventud... La imagen de la mujer sigue apareciendo estereotipada en la publicidad, utilizada como objeto de deseo y mero acompañamiento del producto que se pretende vender. Una construcción de identidades de género que se transmite a los más jóvenes a través de un lenguaje persuasivo, altamente eficaz para la creación de valores. A pesar de las décadas de aplicación de la legislación que expresamente prohíbe la utilización de la imagen de la mujer en el mensaje publicitario desvinculada del producto y la perpetuación de estereotipos de género, la publicidad sexista sigue estando presente, siendo especialmente preocupante en la de productos dirigidos a jóvenes, debido a su carácter persuasivo y su capacidad de transmitir modelos, y en el soporte audiovisual, por la amplia exposición de este target al mismo

Razonamientos no rigurosos y demostraciones asistidas por ordenador

Presentamos la contribución de Th. Tymoczko a la filosofía de la matemática y analizamos y evaluamos las demostraciones asistidas por ordenador y los razonamientos no rigurosos en la matemática experimental, con particular referencia al Teorema de los Cuatro Colores.We present Th. Tymoczko’s contribution to the philosophy of mathematics, and we analyze and evaluate the computer-assisted proofs and the non-rigorous reasonings in the experimental mathematics, particularly in reference to the Four-Colour Theorem

Jet Power in Pre-Planetary Nebulae: Observations vs. Theory

High velocity jets are among the most prominent features of a wide class of planetary nebulae, but their origins are not understood. Several different types of physical model have been suggested to power the jets, but there is no consensus or preferred scenario. We compare current theoretical ideas on jet formation with observations, using the best studied pre-planetary nebulae in millimeter CO, where the dynamical properties are best defined. In addition to the mass, velocity, momentum, and energy of the jets, the mass and energetics of the equatorial mass-loss that typically accompanies jet formation prove to be important diagnostics. Our integrated approach provides estimates for some key physical quantities - such as the binding energy of the envelope when the jets are launched - and allows testing of model features using correlations between parameters. Even with a relatively small sample of well-observed objects, we find that some specific scenarios for powering jets can be ruled out or rendered implausible, and others are promising at a quantitative level.Comment: 4 pages, 1 figure, to appear in "Planetary Nebulae: an Eye to the Future", IAU Symposium 283, eds. A Manchado, L. Stanghellini, D. Schoenberne

Panorama de arquitectura latinoamericana joven. II Bienal de Arquitectura Latinoamericana BAL 2011 en Pamplona

El pasado mes de abril tuvo en lugar la segunda edición de la Bienal de Arquitectura Latinoamericana BAL un evento que se consolida como un lugar de encuentro para los jóvenes arquitectos emergentes a la vez que una excepcional oportunidad de otear el horizonte de lo que se presenta como el futuro de la arquitectura en el continente sudamericano. En esta segunda edición fueron seleccionados para mostrar su trabajo doce jóvenes equipos que convirtieron Pamplona, durante los tres intensos días que duró el evento, en embajadora de la joven arquitectura latinoamericana en España. Con motivo del protagonismo de Chile, país invitado en esta edición, también se inauguró un exposición monográfica sobre arquitectura de ese país, mostrando desde la modernidad más ortodoxa hasta las prácticas contemporáneas más celebradas