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The radiative newtonian 1 < γ ≤ 1.66 and the paczyński–wiita γ = 5/3 regime of non-isothermal bondi accretion onto a massive black hole with an accretion disc
ArticleAbstract: We investigate the non-isothermal Bondi accretion onto a supermassive black hole (SMBH) for the unexPalabras claves:Accretion of matter, Black hole evolution, Galaxies: evolution, galaxies: nuclei, Supermassive black holeAutores:Ernesto Contreras, Gabbasov R., J. M. Ramirez, Klapp J., Sigalotti L.D.G., Sigalotti L.DiG.Fuentes:scopusCreating and using large grids of precalculated model atmospheres for a rapid analysis of stellar spectra
ArticleAbstract: Aims. We present a database of 43 340 atmospheric models (∼80 000 models at the conclusion of the prPalabras claves:methods: data analysis, miscellaneous, Stars: atmospheresAutores:Arias L., Arrieta A., Fierro-Santillán C.R., Hareter M., Klapp J., Raul E. Puebla, Sigalotti L.D.G., Sigalotti L.DiG., Valencia J.M., Zsargó J.Fuentes:googlescopusEfficiency of particle search methods in smoothed particle hydrodynamics: a comparative study (part I)
ArticleAbstract: Nearest neighbour searching is central to the efficiency of smoothed particle hydrodynamics (SPH). HPalabras claves:Closest pair search, Data structures, Nearest neighbour search, Smoothed particle hydrodynamics, SPHAutores:Di Sigalotti L.G., Eric Plaza, FCNM ESPOL, María Castro, Pérez L., Sigalotti L.D.G., Troconis J., Wilfredo AnguloFuentes:googlescopusErratum: Bondi accretion for adiabatic flows onto a massive black hole with an accretion disc: The one dimensional problem (A& A (2019) 631 (A13) DOI: 10.1051/0004-6361/201935917)
OtherAbstract: A more appropriate observational reference for footnote 2 (page 4) of the article is: For warm absorPalabras claves:Autores:Ernesto Contreras, Gabbasov R., J. M. Ramirez, Klapp J., Sigalotti L.D.G., Sigalotti L.DiG.Fuentes:scopus