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...
Massive 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...
Massive 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...
Massive 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...
Massive 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...
Massive galaxies: a gate to large area very deep galaxy surveys
Massive (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...
Massive stars play a key role in environments with very different metallicities. To interpret the role of massive stars in these systems we have to know their...
We are on the cusp of a revolution in massive star research triggered by 2MASS and Spitzer/GLIMPSE, and now is the ideal time to capitalize on these projects by...