NGC 7419 as a template for red supergiant clusters

Context. The open cluster NGC 7419 is known to contain five red supergiants and a very high number of Be stars. However, there are conflicting reports about its age and distance that prevent a useful comparison with other clusters. Aims. We intend to obtain more accurate parameters for NGC 7419, using techniques different from those of previous authors, so that it may be used as a calibrator for more obscured clusters. Methods. We obtained Strömgren photometry of the open cluster NGC 7419, as well as classification spectroscopy of ~20 stars in the area. We then applied standard analysis and classification techniques. Results. We find a distance of 4 ± 0.4 kpc and an age of 14 ± 2 Myr for NGC 7419. The main-sequence turn-off is found at spectral type B1, in excellent agreement. We identify 179 B-type members, implying that there are more than 1200 M⊙ in B stars at present. Extrapolating this to lower masses indicates an initial cluster mass of between 7000 and 10 000 M⊙, depending on the shape of the initial mass function. We find a very high fraction (≈40%) of Be stars around the turn-off, but very few Be stars at lower masses. We also report for the first time a strong variability in the emission characteristics of Be stars. We verified that the parameters of the red supergiant members can be used to obtain accurate cluster parameters. Conclusions. NGC 7419 is sufficiently massive to serve as a testbed for theoretical predictions and as a template to compare more obscured clusters. The distribution of stars above the main-sequence turn-off is difficult to accommodate with current evolutionary tracks. Though the presence of five red supergiants is marginally consistent with theoretical expectations, the high number of Be stars and very low number of luminous evolved B stars hint at some unknown physical factor that is not considered in current synthesis models.

Computer Networks Virtualization with GNS3: Evaluating a solution to optimize resources and achieve a distance learning

Designing educational resources allow students to modify their learning process. In particular, on-line and downloadable educational resources have been successfully used in engineering education the last years [1]. Usually, these resources are free and accessible from web. In addition, they are designed and developed by lecturers and used by their students. But, they are rarely developed by students in order to be used by other students. In this work-in-progress, lecturers and students are working together to implement educational resources, which can be used by students to improve the learning process of computer networks subject in engineering studies. In particular, network topologies to model LAN (Local Area Network) and MAN (Metropolitan Area Network) are virtualized in order to simulate the behavior of the links and nodes when they are interconnected with different physical and logical design.

Virtualización de Redes de Computadores con GNS3: Evaluación de soluciones para el aprendizaje a distancia

El diseño de los recursos educativos permite a los estudiantes modificar su proceso de aprendizaje. En particular, los recursos educativos on-line descargables han sido utilizados con éxito en la educación en ingeniería en los últimos años. Por lo general, estos recursos son gratuitos y accesibles desde la web. Además, son diseñados y desarrollados por profesores y usados por sus estudiantes. Pero, rara vez se desarrollan por los estudiantes con el fin de ser utilizados por otros estudiantes. En este artículo, profesores y estudiantes trabajan juntos para implementar recursos educativos de libre distribución, que puedan ser utilizados por los estudiantes para mejorar el proceso de aprendizaje de redes de computadores en los estudios de ingeniería. En particular, se virtualizan topologías de red para modelar redes LAN (Local Area Network) y MAN (Metropolitan Area Network) con el fin de simular el comportamiento de los enlaces y nodos cuando están interconectados con diferente diseño físico y lógico. Para ello, usando el software de libre distribución GNS3, y teniendo como base la configuración de la red del laboratorio L24 de la EPS, se construye un entorno virtual que simula las posibilidades reales de este laboratorio.