Search Results - "Oreiro, R."

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  1. 1

    Analysis of the rich frequency spectrum of KIC 10670103 revealing the most slowly rotating subdwarf B star in the Kepler field by Reed, M. D., Foster, H., Telting, J. H., Østensen, R. H., Farris, L. H., Oreiro, R., Baran, A. S.

    “…We analyse 2.75 yr of Kepler spacecraft observations of the pulsating subdwarf B star KIC 10670103. These 1.4 million measurements have an impressive duty…”
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    Journal Article
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    Identification of new hot subdwarf binary systems by means of Virtual Observatory tools by Solano, E, Ulla, A, Pérez-Fernández, E, Rodrigo, C, Oreiro, R, Aller, A, Manteiga, M, Santoveña-Gómez, R, Álvarez, M A, Dafonte, C

    “…ABSTRACT The estimation of the binary fraction of hot subdwarfs is key to shed light on the different evolution scenarios proposed to explain the loss of the…”
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    A search for new hot subdwarf stars by means of virtual observatory tools II by Pérez-Fernández, E., Ulla, A., Solano, E., Oreiro, R., Rodrigo, C.

    “…Recent massive sky surveys in different bandwidths are providing new opportunities to modern astronomy. The Virtual Observatory (VO) represents the adequate…”
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    The physical structure of planetary nebulae around sdO stars: Abell 36, DeHt 2, and RWT 152 by Aller, A, Miranda, L F, Olguin, L, Vazquez, R, Guillen, P F, Oreiro, R, Ulla, A, Solano, E

    “…We present narrow-band Hα and [O iii] images, and high-resolution, long-slit spectra of the planetary nebulae (PNe) Abell 36, DeHt 2, and RWT 152 aimed at…”
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    J08069+1527: a newly discovered high-amplitude, hybrid subdwarf B pulsator by Baran, A. S., Gilker, J. T., Reed, M. D., Østensen, R. H., Telting, J. H., Smolders, K., Hicks, L., Oreiro, R.

    “…We present our discovery of a new hybrid pulsating subdwarf B (sdB) star, J08069+1527. The effective temperature and surface gravity of 28 500 ± 400 K and 5.37…”
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    Study of sdO models: pulsation analysis by Rodríguez-López, C., Moya, A., Garrido, R., MacDonald, J., Oreiro, R., Ulla, A.

    “…We have explored the possibility of driving pulsation modes in models of subluminous O-stars (sdOs), in which the effects of element diffusion, gravitational…”
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    Study of sdO models: mode trapping by Rodríguez-López, C., Moya, A., Garrido, R., MacDonald, J., Oreiro, R., Ulla, A.

    “…We present the first description of mode trapping for subdwarf O (sdO) models. Mode trapping of gravity modes caused by the He/H chemical transition is found…”
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    Time-resolved high-resolution spectroscopy of the pulsating sdB star QQ Vir (PG1325+101) by Telting, J., Østensen, R., Oreiro, R., Heber, U., Vučković, M., Randall, S., Baran, A.

    Published in Astrophysics and space science (01-10-2010)
    “…In March 2008 we obtained 2 nights of time-resolved high-resolution spectroscopy with UVES@VLT of the pulsating sdB QQ Vir (PG1325+101), totalling more than…”
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    Mode trapping in sdO models by Rodríguez-López, C., Moya, A., Garrido, R., MacDonald, J., Oreiro, R., Ulla, A.

    Published in Astrophysics and space science (01-10-2010)
    “…Mode trapping of high-radial order gravity modes was found for a particular sdO model. The trapping is caused by the change in composition from the helium…”
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    Synthetic pulsational line profile variations by Oreiro, R., Telting, J. H., Østensen, R. H., Briquet, M., Aerts, C., Heber, U., Vučković, M.

    Published in Astrophysics and space science (01-10-2010)
    “…We have produced simulated time series of high resolution spectroscopy for sdBs. We present the first results of testing classical mode identification…”
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    Hot Subdwarfs: Magnetic, Oscillatory and Other Physical Properties by Oreiro, R, Pérez Hernández, F, Manteiga, M, Ulla, A, González Pérez, Jm, Zapatero Osorio, Mr, GarcÍa López, R, Macdonald, J, Thejll, P, Ferriz-mas, A, Saffer, Ra, Elkin, V

    Published in Astrophysics and space science (01-01-2003)
    “…Hot subdwarf stars (hot sds) are blue subluminous objects. Only a few determinations areavailable to date regarding the study of such aspects as…”
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    Journal Article
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