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  • Evolution and CNO yields of Z = 10-5 stars and possible effects on carbon-enhanced metal-poor production

     Gil Pons, Pilar; Doherty, Carolyn L.; Lau, Herbert B.; Campbell, Simon W.; Suda, Takuma; Guilani, Shervin Mansouri; Gutierrez Cabello, Jorge Luis; Lattanzio, John C.
    Astronomy and astrophysics
    Date of publication: 2013-09
    Journal article

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    Aims. Our main goals are to get a deeper insight into the evolution and final fates of intermediate-mass, extremely metal-poor (EMP) stars. We also aim to investigate the C, N, and O yields of these stars. Methods. Using the Monash University Stellar Evolution code MONSTAR we computed and analysed the evolution of stars of metallicity Z = 10-5 and masses between 4 and 9 M¿, from their main sequence until the late thermally pulsing (super) asymptotic giant branch, TP-(S)AGB phase. Results. Our model stars experience a strong C, N, and O envelope enrichment either due to the second dredge-up process, the dredge-out phenomenon, or the third dredge-up early during the TP-(S)AGB phase. Their late evolution is therefore similar to that of higher metallicity objects. When using a standard prescription for the mass loss rates during the TP-(S)AGB phase, the computed stars are able to lose most of their envelopes before their cores reach the Chandrasekhar mass (mCh), so our standard models do not predict the occurrence of SNI1/2 for Z = 10-5 stars. However, we find that the reduction of only one order of magnitude in the mass-loss rates, which are particularly uncertain at this metallicity, would prevent the complete ejection of the envelope, allowing the stars to either explode as an SNI1/2 or become an electron-capture SN. Our calculations stop due to an instability near the base of the convective envelope that hampers further convergence and leaves remnant envelope masses between 0.25 M¿ for our 4 M¿ model and 1.5 M¿ for our 9 M¿ model. We present two sets of C, N, and O yields derived from our full calculations and computed under two different assumptions, namely, that the instability causes a practically instant loss of the remnant envelope or that the stars recover and proceed with further thermal pulses. Conclusions. Our results have implications for the early chemical evolution of the Universe and might provide another piece for the puzzle of the carbon-enhanced EMP star problem.

  • Ciencia en Acción

     Gutierrez Cabello, Jorge Luis; Berenguer Sau, Jordi; de Villardi de Montlaur, Adeline
    Award or recognition

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    Spherical Rover for lunar and planetary exploration  Open access

     Gutierrez Cabello, Jorge Luis; Tristancho Martinez, Joshua
    European Lunar Symposium
    Presentation's date: 2012-04-19
    Presentation of work at congresses

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    Historically, planetary and lunar rovers have been wheeled-driven. While this is usually seen as an advantage –due to the flight experience– in some cases, the unavoidable presence of gears and mobile parts can be a significant hazard to the mission. The abrasive lunar regolith has been the origin of substantial problems with the Apollo rovers. Here we propose a completely different scheme: a spherical rover in which all the moving parts are protected from the environment by an external spherical shell

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    Simplified Femto-satellite Operations for Disaster Management Missions  Open access

     Tristancho Martinez, Joshua; Gutierrez Cabello, Jorge Luis
    International Astronautical Congress
    Presentation's date: 2012-10-02
    Presentation of work at congresses

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    The reduction in size of satellites is reaching at the range of femto-satellites, i.e. satellites less than 100 grams in mass. One of the key points to achieve such a reduc tion is to simplify the design of the satellite, bu t also to simplify their mission operation. In the present work, a sim plified method for responsive femto-satellite opera tions is presented which is able to deal with the main types of disaster management tasks. Then, a mission is e asy to program using a few default functionalities in everyone of a cooperative satellite swarm giving a list of coor dinates. The protocol is able to update the list for adaptive mi ssions which are based on coordinates. This feature would allow an easy control for the first responders when they are in the field in the beginning of an emergency. The se satellites could send real-time pictures to the first responde rs agents, without the need of a complex ground sta tion infrastructure, until the help arrives

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    A comparison of analytical models for resonant inductive coupling wireless power transfer  Open access

     Bou, Elisenda; Alarcon Cot, Eduardo Jose; Gutierrez Cabello, Jorge Luis
    Progress in Electromagnetics Research Symposium
    Presentation's date: 2012
    Presentation of work at congresses

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    Recent research in wireless power transfer (WPT) using resonant inductive coupling has demonstrated very high efficiencies (above 40%) at large distances compared to the antenna dimensions, which has exponentially increased the number of potential applications of WPT. Since resonant inductive coupling is a very multidisciplinary field, different approaches have been proposed to predict the behaviour of these systems from physical theory of resonators, reflected load theory and the circuit point of view. However, the relation between these methods is still obscure. In this article, we compare the results of these models to find the effciency of a Resonant Inductive Coupling WPT system under Steady-State sonditions and to analyze the relation between the optimal load values obtained from this perspectives and the ones obtained using impedance matching techniques.

    Recent research in wireless power transfer (WPT) using resonant inductive coupling has demonstrated very high e±ciencies (above 40%) at large distances compared to the antenna dimensions, which has exponentially increased the number of potential applications of WPT. Since resonant inductive coupling is a very multidisciplinary ¯eld, di®erent approaches have been proposed to predict the behaviour of these systems from physical theory of resonators, reflected load theory and the circuit point of view. However, the relation between these methods is still obscure. In this article, we compare the results of these models to find the effciency of a Resonant Inductive Coupling WPT system under Steady-State sonditions and to analyze the relation between the optimal load values obtained from this perspectives and the ones obtained using impedance matching techniques.

  • Mart XXI o de com anar de la secundària a la universitat passant per Mart

     Almansa Lagunas, Clara; Blay Carreras, Estel; Casas Carbonell, Montserrat; Delgado Muñoz, Luis; Gutierrez Cabello, Jorge Luis; Jove Casulleras, Roger; Lopez Codina, Daniel; López Rubio, Juan; Loren Aguilar, Pablo; Marando, Graciela; Monfort Peligero, Lluís; Nebra, Norbert; Pera, Francesc; Portell Canal, Xavier; Ramírez Alcantara, Jorge; Sagardoy, Juli; Sánchez, Álex
    Date: 2011-11-22
    Report

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  • BUILDING ON THE INTERNATIONAL YEAR OF ASTRONOMY: MAKING YOUNG CHILDREN AWARE OF THE UNIVERSE

     Cors Iglesias, Josep Maria; Ros Ferre, Rosa Maria; Gutierrez Cabello, Jorge Luis; Mazon Bueso, Jordi; Espona Dones, Margarida; Fabregat Fillet, Jaime
    Participation in a competitive project

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  • EU-UNAWE

     Fabregat Fillet, Jaime; Mazon Bueso, Jordi; Gutierrez Cabello, Jorge Luis; Cors Iglesias, Josep Maria
    Participation in a competitive project

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  • A probe of concept for femto-satellites based on commercial-of-the-shelf

     Tristancho Martinez, Joshua; Gutierrez Cabello, Jorge Luis
    Digital Avionics Systems Conference
    Presentation's date: 2011-10-18
    Presentation of work at congresses

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  • Setmana'09 de les Telecomunicacions

     Palà Schönwälder, Pere; Berenguer Sau, Jordi; Esquerra Llucià, Ignasi; Gabriel, JosepMa; Giralt Mas, M. Rosa; Marques Calvo, Jose Joaquin; Gutierrez Cabello, Jorge Luis; del Águila López, Francisco
    Collaboration in exhibitions

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    On the fate of extremely low metallicity stars  Open access

     Gil Pons, Pilar; Gutierrez Cabello, Jorge Luis; Garcia-berro Montilla, Enrique; Althaus, Leandro G.
    AIP Conference proceedings
    Date of publication: 2008
    Journal article

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    We have computed and analyzed the evolution of intermediate-mass stars of metallicity Z = 10−5 from the main sequence until the early stages of the TP-(S)AGB phase. In order to check the influence of mixing we have performed our calculations using two different evolutionary codes, EVOLVE — which does not include diffusion but allows for overshooting— and LPCODE, which includes diffusion and overshooting “à-la-Herwig”. Important differences appear during the TP– AGB phase, as the calculations done with EVOLVE lead to an almost negligible third dredge-up, whereas the sequences computed with LPCODE show important third dredge-up and, therefore, significant enrichment in metals of the envelope. This fact has consequences on the strength of the winds during the TP-AGB phase and, ultimately, on the final fate of the considered stars. Also, the models computed with LPCODE show strong double flashes produced by the ingestion of protons on the helium burning shell.

    Postprint (author’s final draft)

  • On the Fate of Extremely Low Metallicity Stars

     Gil Pons, Pilar; Gutierrez Cabello, Jorge Luis; Garcia-berro Montilla, Enrique; Althaus, Leandro G.
    AIP Conference proceedings
    Date of publication: 2008-12-01
    Journal article

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    Is there a chance for primordial SNeI1/2?  Open access

     Gil Pons, Pilar; Gutierrez Cabello, Jorge Luis; Garcia-berro Montilla, Enrique
    Proceedings of Science
    Date of publication: 2007-09
    Journal article

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    The evolution of primordial stars of initial masses between 5 and 10 M⊙ has been computed and analyzed in order to determine the nature of the remnants of massive intermediate–mass primordial stars and to check the influence of overshooting in their evolution. We have obtained the values for the limiting masses of Population III progenitor stars leading to carbon–oxygen and oxygen–neon compact cores. We have also obtained the limiting mass for which isolated primordial stars would lead to core–collapse supernovae after the end of the main central burning phases. Considering a moderate amount of overshooting, the mass thresholds at the ZAMS for the formation of carbon–oxygen and oxygen–neon degenerate cores shift to smaller values by about 2 M⊙. As a by–product of our calculations, we have also obtained the structure and composition profiles of the resulting compact remnants. We find that the final fate of the considered stars could not be to become white dwarfs, as it is the case of objects of larger metallicity of analogous initial masses. Instead, as we show by means of a synthetic code, they might end their lives as SNI1/2.

  • Is there a chance for SNI1/2?

     Gil Pons, Pilar; Gutierrez Cabello, Jorge Luis; Garcia-berro Montilla, Enrique
    XXIII Trobades científiques de la Mediterrània: supernovae: light in the darkness
    Presentation of work at congresses

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  • On the fate of extremely low metallicity stars

     Gil Pons, Pilar; Gutierrez Cabello, Jorge Luis; Garcia-berro Montilla, Enrique; Althaus, Leandro Gabriel
    IXth Torino Workshop on Evolution and Nucleosynthesis in AGB Stars; II Perugia Workshop on Nuclear Astrophysics
    Presentation of work at congresses

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  • Is there a chance for primordial SNI1/2?

     Gil Pons, Pilar; Gutierrez Cabello, Jorge Luis; Garcia-berro Montilla, Enrique
    Fisrt stars III
    Presentation of work at congresses

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  • Is there a chance for SNI1/2?

     Gutierrez Cabello, Jorge Luis
    XXIII Trobades científiques de la Mediterrània: supernovae: light in the darkness
    Presentation's date: 2007-10-03
    Presentation of work at congresses

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  • The Late stages of the evolution of intermediate-mass primordial stars: The effects of overshooting

     Gil Pons, Pilar; Gutierrez Cabello, Jorge Luis; Garcia-berro Montilla, Enrique
    Astronomy and astrophysics
    Date of publication: 2007-03
    Journal article

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  • The Degenerate remmant cores of ultra-metal-poor-heavy-weight intermediate mass stars: white dwarfs or supernovae?

     Garcia-berro Montilla, Enrique; Gil Pons, Pilar; Gutierrez Cabello, Jorge Luis
    15th European Workshop on White Dwarfs
    Presentation of work at congresses

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  • The degenerate remnant cores of ultra-metal-poor heavy-weight intermediate-mass stars: white dwarfs of supernovae?

     Garcia-berro Montilla, Enrique; Gil Pons, Pilar; Gutierrez Cabello, Jorge Luis
    15th European Workshop on White Dwarfs
    Presentation of work at congresses

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  • Did intermediate-mass primordial stars explode as SNeI.5?

     Gutierrez Cabello, Jorge Luis
    Supernovae:one millenium after SN1006?
    Presentation's date: 2006-05-16
    Presentation of work at congresses

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  • The Evolution of primordial Super-AGB stars

     Garcia-berro Montilla, Enrique; Gil Pons, Pilar; Gutierrez Cabello, Jorge Luis
    Memorie della Societá Astronomica Italiana
    Date of publication: 2006-08
    Journal article

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  • The gravitational collapse of ONe electron-degenerate cores and white dwarfs: the role of 24Mg and 12C revisited

     Gutierrez Cabello, Jorge Luis; Garcia-berro Montilla, Enrique
    Astronomy and astrophysics
    Date of publication: 2005-03
    Journal article

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  • Evolución Final de objetos degenerados de ONe(Mg)

     Gutierrez Cabello, Jorge Luis
    Defense's date: 2002-12-19
    UB
    Theses

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  • Contrapartidas ópticas de fuentes explosivas de rayos gamma

     Gutierrez Cabello, Jorge Luis
    Date of publication: 2002-05-31
    Book chapter

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  • Europa: ¿Mareas, océano, vida?

     Gutierrez Cabello, Jorge Luis
    Date of publication: 2002-05-31
    Book chapter

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  • Las supernovas

     Gutierrez Cabello, Jorge Luis
    Date of publication: 2002-05-31
    Book chapter

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  • El cosmos

     Estalella Boadella, Robert; Asiain, R; Galadí, D; Gutierrez Cabello, Jorge Luis; Prades, A; Ribas, I; Sepúlveda, I
    Date of publication: 2002-05-31
    Book

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  • Terrene meteorites on the Moon

     Gutierrez Cabello, Jorge Luis
    Date of publication: 2001-06-30
    Book chapter

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  • Astronomía general. teoría y práctica

     Gutierrez Cabello, Jorge Luis
    Date of publication: 2001-03-31
    Book

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  • SIXE: An X-ray experiment for the MINISAT platform

     Isern Vilaboy, Jordi; Giovanelli, F.; Sabau, L.; Bravo Guil, Eduardo; Gomez-Gomar, J.; Hernanz Carbó, Margarita; Garcia-berro Montilla, Enrique; La Padula, C.D.; Gutierrez Cabello, Jorge Luis; José Pont, Jordi; Garcia Senz, Domingo; Bausells Roigé, Joan; Cabestany Moncusi, Joan; Madrenas Boadas, Jordi; Angulo, M.; Fernandez-Valbuena, M.; Herrera, E.; Reina, M.; Talavera, A.
    Astrophysics and space science
    Date of publication: 2001-01
    Journal article

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    SIXE (Spanish Italian X-ray Experiment) is an X-ray payload with geometric area of ~3200 cm2 , formed by four identical gas-filled Multiwire Proportional Counters devoted for a long term spectroscopy of selected X-ray sources in the energy range ~3-60 KeV. The spectral resolution of ~5% for E>35 KeV and ¿E/E=60/E1/2 for E<35 KeV, the continuum sensitivity (3o in 105 s) of ~3¿10-6ph/cm2 ¿KeV, the line detection sensitivity (3o in 105 s) of ~3.5¿10-6ph /cm2 ¿KeV, the time accuracy of 0.1 ms, the experiment weight of ~90 Kg, the full dimensions including the electronic box of ~660x660x400 mm3, the power budget of -40 W, the telemetry rate of :=100 Kbit/s and on-board memory of ~2 Gbytes makes this experiment fully compatible for a minisatellite mission, such as for istance the spanish MINISAT 02. The main scientific goal of SIXE is the study of the short and long term spectral and intensity variabilities of few selected extragalactic and galactic X-ray sources, such as quasars, Seyfert galaxies, high and low mass X-ray binaries, etc. Since the sensitivity and the energy resolution of SIXE are rather good, it is possible to study the behaviour of the eventual Fe lines with respect to the continuum emission. This possibility of SIXE is unique for the present generation of X-ray experiments, since no one is dedicated to long term monitoring of X-ray sources.

    SIXE (Spanish Italian X-ray Experiment) is an X-ray payload with geometric area of ~3200 cm2 , formed by four identical gas-filled Multiwire Proportional Counters devoted for a long term spectroscopy of selected X-ray sources in the energy range ~3-60 KeV. The spectral resolution of ~5% for E>35 KeV and ¿E/E=60/E1/2 for E<35 KeV, the continuum sensitivity (3o in 105 s) of ~3•10-6ph/cm2 •KeV, the line detection sensitivity (3o in 105 s) of ~3.5•10-6ph /cm2 •KeV, the time accuracy of 0.1 ms, the experiment weight of ~90 Kg, the full dimensions including the electronic box of ~660x660x400 mm3, the power budget of -40 W, the telemetry rate of :=100 Kbit/s and on-board memory of ~2 Gbytes makes this experiment fully compatible for a minisatellite mission, such as for istance the spanish MINISAT 02. The main scientific goal of SIXE is the study of the short and long term spectral and intensity variabilities of few selected extragalactic and galactic X-ray sources, such as quasars, Seyfert galaxies, high and low mass X-ray binaries, etc. Since the sensitivity and the energy resolution of SIXE are rather good, it is possible to study the behaviour of the eventual Fe lines with respect to the continuum emission. This possibility of SIXE is unique for the present generation of X-ray experiments, since no one is dedicated to long term monitoring of X-ray sources.

  • Terrene meteorites on the Moon

     Gutierrez Cabello, Jorge Luis
    First Steps in the Origin of Life in the Universe
    Presentation of work at congresses

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  • Terrene meteorites on the Moon

     Gutierrez Cabello, Jorge Luis
    First Steps in the Origin of Life in the Universe
    Presentation's date: 2000-09-03
    Presentation of work at congresses

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  • SIXE: An X-ray mission for a minisatellite

     Isern Vilaboy, Jorge; Bravo Guil, Eduardo; Gómez Gomar, J.; Hernanz Carbó, Margarita; Garcia-berro Montilla, Enrique; Gutierrez Cabello, Jorge Luis; José Pont, Jordi; Garcia Senz, Domingo; Cabestany Moncusi, Joan; Madrenas Boadas, Jordi
    Small Missions for Energetic Astrophysics
    Presentation of work at congresses

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  • Spanish-Italian X-ray Experiment: Feasibility Study Report

     Isern Vilaboy, Jorge; Bravo Guil, Eduardo; Gómez Gomar, J.; Garcia-berro Montilla, Enrique; Giovannelli, F; Padula, C. de la; Sabau, L.; Hernanz Carbó, Margarita; Madrenas Boadas, Jordi; Gutierrez Cabello, Jorge Luis; José Pont, Jordi; Garcia Senz, Domingo; Badenes Montoliu, Carles; Bausells Roigé, Joan; Cabestany Moncusi, Joan; Fernández Valbuena, M.; Herrera, M.; Reina, M.; Talavera, A.
    Date: 1999-03
    Report

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  • SIXE feasibility Study: Work Package Description: Ground and User Segment

     Garcia-berro Montilla, Enrique; Gutierrez Cabello, Jorge Luis
    Date: 1998-01
    Report

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  • SIXE feasibility study. Final report

     Isern Vilaboy, Jorge; Bravo Guil, Eduardo; Gómez Gomar, J.; Hernanz Carbó, Margarita; Garcia-berro Montilla, Enrique; Gutierrez Cabello, Jorge Luis; José, J.; Garcia Senz, Domingo; Badenes Montoliu, Carles; Ganzo, F; Llano, R. del; Giovannelli, F; Padula, C. de la; Frutti, M.; Sabau, L.; Fernández Valbuena, M.; Herrera Cañadas, Eloi; Reina, M.; Talavera, A.; Cabestany Moncusi, Joan; Madrenas Boadas, Jordi; Bausells Roigé, Joan
    Date: 1998-08
    Report

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  • SIXE Feasibility Study. Ground and User segment: SIXE Scientific Committee

     Garcia-berro Montilla, Enrique; Gutierrez Cabello, Jorge Luis
    Date: 1998-07
    Report

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  • SIXE Feasibility Study. Ground and User segment: Data Processing and Archiving Center

     Garcia-berro Montilla, Enrique; Gutierrez Cabello, Jorge Luis
    Date: 1998-07
    Report

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  • SIXE Feasibility Study. Ground and User segment: The Scientific Operations Planning Center

     Garcia-berro Montilla, Enrique; Gutierrez Cabello, Jorge Luis
    Date: 1998-07
    Report

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  • SIXE Feasibility Study. Ground and User segment: Telemetry and Telecommand

     Garcia-berro Montilla, Enrique; Gutierrez Cabello, Jorge Luis
    Date: 1998-04
    Report

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  • SIXE Feasibility Study. Ground and User segment: Mission Control Center

     Garcia-berro Montilla, Enrique; Gutierrez Cabello, Jorge Luis
    Date: 1998-04
    Report

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  • SIXE Feasibility Study. Ground and User segment: General Overview

     Garcia-berro Montilla, Enrique; Gutierrez Cabello, Jorge Luis
    Date: 1998-07
    Report

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  • SIXE: Spanish-Italian X-ray Experiment. Feasibility Study Report

     Isern Vilaboy, Jorge; Bravo Guil, Eduardo; Gómez Gomar, J.; Garcia-berro Montilla, Enrique; Giovannelli, F; Padula, C. de la; Sabau, L.; Gutierrez Cabello, Jorge Luis; José Pont, Jordi; Hernanz Carbó, Margarita; Garcia Senz, Domingo; Badenes Montoliu, Carles; Bausells Roigé, Joan; Cabestany Moncusi, Joan; Madrenas Boadas, Jordi; Fernández Valbuena, M.; Herrera, M.; Reina, M.; Talavera, A.
    Date: 1998-08
    Report

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  • SIXE Feasibility Study. Work Package Description: Ground and User segment.

     Garcia-berro Montilla, Enrique; Gutierrez Cabello, Jorge Luis
    Date: 1997-11
    Report

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  • Final Evolution of 8-10 M. stars

     Gutierrez Cabello, Jorge Luis; Garcia-berro Montilla, Enrique
    Date of publication: 1996-10
    Book chapter

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  • The final evolution of O-Ne-Mg electron-degenerate cores

     Gutierrez Cabello, Jorge Luis; Garcia-berro Montilla, Enrique
    Astrophysical journal
    Date of publication: 1996-03
    Journal article

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  • The final evolution of 8-10 M. stars

     Gutierrez Cabello, Jorge Luis; Ramon, Canal; Javier, Labay; Jordi, Isern; Garcia-berro Montilla, Enrique
    NATO Advanced Study Institute on Thermonuclear Supernovae
    Presentation of work at congresses

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  • The Final Fate of 8-10 Solar Masses Stars

     Gutierrez Cabello, Jorge Luis
    Date of publication: 1995-12-01
    Book chapter

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