Post T Tauri stars in the solar neighborhood: isolated or members of young associations and moving groups

Post T Tauri stars (PTTS) are late-type stars in the age range between 10 and 100 Myr filling the gap between T Tauri (TTs) and zero-age: main sequence phases. This period of evolution remains ambiguous and until now different studies of young stars have failed to find the numbers of PTTS that are expected. In the last years, some PTTS have been identified among the X-ray detected pre-main sequence stars in some star-forming regions. More recently, additional PTTS have been identified in young associations and moving groups (β Pic, TW Hya, Tucana/Horologium, and the AB Dor). However, many isolated PTTS still remain undiscovered. In this contribution, we compiled the PTTS previously identified in the literature, and identified new candidates using the information provided by the high resolution spectra obtained during our surveys of late-type stars possible members to young moving groups, FGK stars in the solar neighborhood, and RasTyc sample. To identify PTTS we applied an age-oriented definition using relative age indicators (Li abundance, chromospheric and coronal emission and the kinematics) as well as color-magnitude diagrams and pre-main sequence isochrones.

Modeling nonthermal emission from stellar bow shocks (Research Note)

Context. Runaway O- and early B-type stars passing through the interstellar medium at supersonic velocities and characterized by strong stellar winds may produce bow shocks that can serve as particle acceleration sites. Previous theoretical models predict the production of high-energy photons by nonthermal radiative processes, but their efficiency is still debated. Aims. We aim to test and explain the possibility of emission from the bow shocks formed by runaway stars traveling through the interstellar medium by using previous theoretical models. Methods. We applied our model to AE Aurigae, the first reported star with an X-ray detected bow shock, to BD+43 3654, in which the observations failed in detecting high-energy emission, and to the transition phase of a supergiant star in the late stages of its life. Results. From our analysis, we confirm that the X-ray emission from the bow shock produced by AE Aurigae can be explained by inverse Compton processes involving the infrared photons of the heated dust. We also predict low high-energy flux emission from the bow shock produced by BD+43 3654, and the possibility of high-energy emission from the bow shock formed by a supergiant star during the transition phase from blue to red supergiant. Conclusions. Bow shocks formed by different types of runaway stars are revealed as a new possible source of high-energy photons in our neighborhood.

Modeling nonthermal emission from stellar bow shocks (Research Note)

Context. Runaway O- and early B-type stars passing through the interstellar medium at supersonic velocities and characterized by strong stellar winds may produce bow shocks that can serve as particle acceleration sites. Previous theoretical models predict the production of high-energy photons by nonthermal radiative processes, but their efficiency is still debated. Aims. We aim to test and explain the possibility of emission from the bow shocks formed by runaway stars traveling through the interstellar medium by using previous theoretical models. Methods. We applied our model to AE Aurigae, the first reported star with an X-ray detected bow shock, to BD+43 3654, in which the observations failed in detecting high-energy emission, and to the transition phase of a supergiant star in the late stages of its life. Results. From our analysis, we confirm that the X-ray emission from the bow shock produced by AE Aurigae can be explained by inverse Compton processes involving the infrared photons of the heated dust. We also predict low high-energy flux emission from the bow shock produced by BD+43 3654, and the possibility of high-energy emission from the bow shock formed by a supergiant star during the transition phase from blue to red supergiant. Conclusions. Bow shocks formed by different types of runaway stars are revealed as a new possible source of high-energy photons in our neighborhood.

Tratado completo de aritmética o Método para aprender a contar por principios : obra útil á toda especie de personas ... /

Mode of access: Internet.

Nueva guía de caminos para ir desde Madrid á todas las Ciudades y Villas más principales de España y Portugal y tambien para ir de unas Ciudades á otras /

Mode of access: Internet.

An X-ray study of the SNR G344.7-0.1 and the central object CXOU J170357.8-414302

Aims. We report results of an X-ray study of the supernova remnant (SNR) G344.7-0.1 and the point-like X-ray source located at the geometrical center of the SNR radio structure. Methods. The morphology and spectral properties of the remnant and the central X-ray point-like source were studied using data from the XMM-Newton and Chandra satellites. Archival radio data and infrared Spitzer observations at 8 and 24 mu m were used to compare and study its multi-band properties at different wavelengths. Results. The XMM-Newton and Chandra observations reveal that the overall X-ray emission of G344.7-0.1 is extended and correlates very well with regions of bright radio and infrared emission. The X-ray spectrum is dominated by prominent atomic emission lines. These characteristics suggest that the X-ray emission originated in a thin thermal plasma, whose radiation is represented well by a plane-parallel shock plasma model (PSHOCK). Our study favors the scenario in which G344.7-0.1 is a 6 x 10^3 year old SNR expanding in a medium with a high density gradient and is most likely encountering a molecular cloud on the western side. In addition, we report the discovery of a soft point-like X-ray source located at the geometrical center of the radio SNR structure. The object presents some characteristics of the so-called compact central objects (CCO). However, its neutral hydrogen absorption column (N_H) is inconsistent with that of the SNR. Coincident with the position of the source, we found infrared and optical objects with typical early-K star characteristics. The X-ray source may be a foreground star or the CCO associated with the SNR. If this latter possibility were confirmed, the point-like source would be the farthest CCO detected so far and the eighth member of the new population of isolated and weakly magnetized neutron stars.

From "ecological tourism" to "ecotourism": lexical analysis of an emerging tourism

From ecological tourism to ecotourism: lexical analysis of an emerging tourism. This article deals with the lexicon created in connection with a recent form of tourism: the ecological tourism or ecotourism. The rise of this type of tourism encourages the creation of new concepts and products that are named with new words and expressions with different procedures of formation. From the name itself ecotourism, then expressed as the acronym ecotourism, we analyze the formation of other related words, as well as their formal variation and use. For this, we have worked with a specific corpus of electronic tourist texts and different digital sources and databases.

Finanzas y modelación

Al igual que las ediciones anteriores, esta publicación compila trabajos de investigación enmarcados en las líneas de trabajos de la Ingeniería Financiera, tanto académicos como aplicados, abarcando las áreas de Riesgos Financieros, Finanzas corporativas y mercado financieros, y aplicando herramientas propias de la Ingeniería Financiera como la econometría financiera, los métodos de valoración de activos, la evaluación del riesgo y aplicaciones en temas tan específicos como el project financey y las finanzas conductuales. Con este libro, además de consolidar la publicación y dar la bienvenida a autores externos de la Universidad, se espera que se pueda impactar no solamente en el ámbito académico sino también en el profesional, y que sirva de material de consulta y referencia para aplicaciones prácticas de temáticas relacionadas con la Ingeniería Financiera a nivel académico y empresarial.

María Estela Guevara de Álvarez (ed.). Antología gnómica de la literatura griega. Líricos arcaicos (poetas elegíacos y yambógrafos). Trad. de G. Barandica, C. Silventi, E. Driban, L. Sardi de Estrella, S. Aguirre de Zárate, P. Arias, M. Fernández Nuin, C. López. Buenos Aires, Santiago Arcos editor, 2014, 160 pp.

Fil: Salatino de Zubiría, María Cristina. Universidad Nacional de Cuyo

[¿Cuáles son los caracteres diferenciales de la monomanía y de la pasión?] : discurso pronunciado ante el claustro de la Universidad Central por el Licenciado en Medicina y Cirujía Don Santiago López Argüeta y Landete, en el acto de recibir la investidura de Doctor en la misma Facultad.

Mode of access: Internet.

Ictiología continental argentina: Santiago del Estero, Catamarca, Córdoba, San Luis, La Pampa y Buenos Aires.

Se presenta un compendio de la información disponible sobre la ictiofauna de parte de la región central de la Argentina y de la provincia de Buenos Aires, así como datos sobre aspectos hidrográficos e ictiogeográficos.