Zobrazeno 1 - 10
of 92
pro vyhledávání: '"Erwin Sedlmayr"'
Publikováno v:
Stock, Joachim W; Kitzmann, Daniel; Patzer, A Beate C; Sedlmayr, Erwin (2018). FastChem: A computer program for efficient complex chemical equilibrium calculations in the neutral/ionized gas phase with applications to stellar and planetary atmospheres (In Press). Monthly notices of the Royal Astronomical Society, 479(1), pp. 865-874. Oxford University Press 10.1093/mnras/sty1531
For the calculation of complex neutral/ionized gas phase chemical equilibria, we present a semi-analytical versatile and efficient computer program, called FastChem. The applied method is based on the solution of a system of coupled nonlinear (and li
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5f68648d4b3a4d3f90dca4d22fa5a086
Autor:
Hans-Peter Gail, Erwin Sedlmayr
Publikováno v:
Physics and Chemistry of Circumstellar Dust Shells
Autor:
Hans-Peter Gail, Erwin Sedlmayr
Publikováno v:
Physics and Chemistry of Circumstellar Dust Shells
Autor:
Hans-Peter Gail, Erwin Sedlmayr
Publikováno v:
Physics and Chemistry of Circumstellar Dust Shells
Publikováno v:
Indian Journal of Physics. 86:555-561
We have theoretically investigated a number of cyclic molecules of four kinds: XC2H2, XC2H4, XC2, and HXC2, where X can be C, N, O, Na, Mg, Al, Si, P, S, and Ca, respectively, which might be present in interstellar and/or circumstellar space, and cal
Publikováno v:
Astronomy & Astrophysics. 499:765-771
Context. Miras and long-period variables (LPVs) are radially pulsating, highly evolved stars on the Asymptotic Giant Branch. Because of peculiar conditions of this objects, their cool, extended atmospheres are ideal sites for the formation of dust pa
Publikováno v:
Astronomy & Astrophysics. 491:643-662
Context. Dust formation, i.e. the condensation of solid particles from a gas phase, occurs in astrophysical environments that are sufficiently cool and offer a sufficiently high density of condensable species. Since many astrophysical systems in whic
Publikováno v:
Astronomy & Astrophysics. 486:497-504
We investigate the mass loss of highly evolved, low- and intermediate mass stars and stellar samples with subsolar metallicity. We give a qualitative as well as quantitative description which can be applied to LMC/SMC-type stellar populations. For th
Autor:
Hans-Peter Gail, Erwin Sedlmayr
Circumstellar dust, the astronomical dust that forms around a star, provides today's researchers with important clues for understanding how the Universe has evolved. This volume examines the structure, dynamics and observable consequences of the dust