664 citations · 2k across the 51 of their papers we have counts for
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Unveiling shocks in planetary nebulae
M. A. Guerrero, J. A. Toalá, J. J. Medina +4
The propagation of a shock wave into a medium is expected to heat the material beyond the shock, producing noticeable effects in intensity line ratios such as [O III]/Halpha. To in…
Crucial aspects of the initial mass function (II): The inference of total quantities from partial information on a cluster
Miguel Cervino, Carlos Romann-Zuniga, Amelia Bayo +3
In a probabilistic framework of the interpretation of the initial mass function (IMF), the IMF cannot be arbitrarily normalized to the total mass, M, or number of stars, N, of the…
Crucial aspects of the initial mass function (I): The statistical correlation between the total mass of an ensemble of stars and its most massive star
Miguel Cervino, Carlos Romann-Zuniga, Valentina Luridiana +3
Our understanding of stellar systems depends on the adopted interpretation of the IMF, phi(m). Unfortunately, there is not a common interpretation of the IMF, which leads to differ…