The San Pedro Mártir Kinematic Catalogue of Galactic Planetary Nebulae

No obstante, como esta enfermedad afecta a cada persona de manera diferente, no todas las opciones de cuidado y tratamiento pueden ser apropiadas para cada individuo.. La forma

Given an accretion rate, and assuming a type I migration rate, one can compute the amount of migration a planet suffers while growing to a gap opening mass.. In thin discs

XXVIII Canary Islands Winter School of Astrophysics – Solar System Exploration Planetary Atmospheres – 3.. Atmospheric dynamics and

These data collectively show PN spectra with thermal dust continua, nebular emission lines, and a variety of dust signatures, with characteristics of carbon-rich and

Altogether, the sample of the 15 most Li-rich giants in the PTPS sample contains three planetary-mass companions (one in a binary system), two possible planetary-mass companions,

Our high- resolution images clearly show that the H 2 emission is not uniformly distributed in a torus around the central star as it has been interpreted from previous

Our interpretation is that the broad infrared features at 6–9, 9–13, 15–20, and 25–35 μm are intimately related with the formation of fullerenes in PNe, being likely produced by

A similar effect is found also for some of the cells with density exceeding the virial mean density (  ≈ 340 for the cosmological parameters assumed here), which are classified