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Toloza Castillo, Odette Fabiola
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Nombre
Toloza Castillo, Odette Fabiola
Departamento
Campus / Sede
Campus Casa Central Valparaíso
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ORCID
Scopus Author ID
36012227500
2 results
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- PublicationTesting Lyα Emission-line Reconstruction Routines at Multiple Velocities in One System(2022-09-01)
;Wilson, David J. ;Youngblood, Allison; ;Drake, Jeremy J. ;France, Kevin ;Froning, Cynthia S. ;Gänsicke, Boris T. ;Redfield, SethWood, Brian E.Abstract The 1215.67 Å H i Lyα emission line dominates the ultraviolet flux of low-mass stars, including the majority of known exoplanet hosts. Unfortunately, strong attenuation by the interstellar medium (ISM) obscures the line core in most stars, requiring the intrinsic Lyα flux to be reconstructed based on fits to the line wings. We present a test of the widely used Lyα emission-line reconstruction code lyapy using phase-resolved, medium-resolution STIS G140M observations of the close white dwarf–M dwarf binary EG UMa. The Doppler shifts induced by the binary orbital motion move the Lyα emission line in and out of the region of strong ISM attenuation. Reconstructions of each spectrum should produce the same Lyα profile regardless of phase, under the well-justified assumption that there is no intrinsic line variability between observations. Instead, we find that the reconstructions underestimate the Lyα flux by almost a factor of 2 for the lowest velocity, most attenuated spectrum, due to a degeneracy between the intrinsic Lyα and ISM profiles. Our results imply that many stellar Lyα fluxes derived from G140M spectra reported in the literature may be underestimated, with potential consequences for, for example, estimates of extreme-ultraviolet stellar spectra and ultraviolet inputs into simulations of exoplanet atmospheres.Scopus© Citations 2 - PublicationA planetesimal orbiting within the debris disc around a white dwarf star(2019-04-05)
;Manser, Christopher J. ;Gänsicke, Boris T. ;Eggl, Siegfried ;Hollands, Mark ;Izquierdo, Paula ;Koester, Detlev ;Landstreet, John D. ;Lyra, Wladimir ;Marsh, Thomas R. ;Meru, Farzana ;Mustill, Alexander J. ;Rodríguez-Gil, Pablo; ;Veras, Dimitri ;Wilson, David J. ;Burleigh, Matthew R. ;Davies, Melvyn B. ;Farihi, Jay ;Fusillo, Nicola Gentile ;de Martino, Domitilla ;Parsons, Steven G. ;Quirrenbach, Andreas ;Raddi, Roberto ;Reffert, Sabine ;Santo, Melania Del ;Schreiber, Matthias R. ;Silvotti, Roberto ;Toonen, Silvia ;Villaver, Eva ;Wyatt, Mark ;Xu, SiyiZwart, Simon PortegiesA low-mass planet around a white dwarf Numerous exoplanets have been detected around Sun-like stars. These stars end their lives as white dwarfs, which should inherit any surviving planetary systems. Manser et al. found periodic shifts in emission lines from a disc of gas orbiting around a white dwarf (see the Perspective by Fossati). They used numerical simulations to show that the most likely explanation for the spectral shifts is a low-mass planet orbiting within the disc. The planet must be unusually small and dense to avoid being ripped apart by tidal forces. The authors speculate that it may be the leftover core of a planet whose outer layers have been removed. Science , this issue p. 66 ; see also p. 25Scopus© Citations 115