Publicación
Mass loss from an extreme OH/IR star: OH 26.5+0.6
Observations of H2O isotopologues of the extreme OH/IR star OH 26.5+0.6 show that the star has an initial mass consistent with it being an intermediate-mass...
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PublicaciónMass Loss in Galactic Globulars: Red Giant Stragglers and Helium White DwarfsThe evolution of Population II Red Giants has been studied by adopting Reimers' formalism for the efficiency of mass loss. Evolutionary computations for models...
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PublicaciónMass, metallicity and SFR relationships in star forming galaxies using deep surveysNot Available
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PublicaciónMassive AGB Stars in the Early Solar System?We present evidence that recently identified massive rubidium-rich AGB stars also played an important role as sources of certain long-lived and short-lived...
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PublicaciónMassive characterisation of subgiants and red giants with TESS (Kepler and Gaia)TESS serves as a formidable tool for investigating stellar variability. Nonetheless, the adaptation of methodologies employed in other space missions, such as...
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PublicaciónMassive compact galaxies in the local Universe: what are they?Recent investigations have provided evidences that many massive (M_* > 10^{11} M_&sun;) spheroid galaxies in the early universe (z ≥ 1.5) were extremely compact...
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PublicaciónMassive galaxies in Extended Groth Strip (Trujillo+, 2007)We use the Palomar Observatory Wide-field Infrared (POWIR)/DEEP-2 survey (Davis et al., 2003, SPIE, Vol. 4834, p. 161; Bundy et al., 2006ApJ...651..120B...
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PublicaciónMassive galaxies in Extended Groth Strip (Trujillo+, 2007)We use the Palomar Observatory Wide-field Infrared (POWIR)/DEEP-2 survey (Davis et al., 2003, SPIE, Vol. 4834, p. 161; Bundy et al., 2006ApJ...651..120B...
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PublicaciónMassive galaxies: a gate to large area very deep galaxy surveysMassive (M_{stellar}≥10^{11} h_{70}^{-2} {M}_{&sun;}) galaxies are privileged probes to explore galaxy evolution, as their high luminosities allow us to track...