Titlebook: Galactic Bulges; Proceedings of the 1 Herwig Dejonghe,Harm J. Habing Conference proceedings 1993 Kluwer Academic Publishers 1993 Bulge.Gala

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新奇

Monte Carlo Simulation Using VHDL-AMSevealed by each type of survey is discussed. Particular attention is given to surveys of the Sgr I clear field, its content of long-period variables and their implications for distance determination and the high end of the Bulge luminosity function.

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overrule

https://doi.org/10.1007/978-94-011-0922-2Bulge; Galaxy; Variation; galaxies; milky way

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978-0-7923-2425-6Kluwer Academic Publishers 1993

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Galactic Bulges978-94-011-0922-2Series ISSN 1743-9213 Series E-ISSN 2352-2186

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Tim Mould MD, FRCOG, MBBS, MA, DM, FRCOGThe available kinematical data on OH/IR stars is discussed, and dynamical models for the OH/IR stars are presented.

foliage

J. Struyven,G. Kuhn,C. C. SchulmanAfter a discussion of the methods used to derive the physical parameters of planetary nebulae and their central stars, the global properties of planetary nebulae in the Galactic bulge are reviewed, and compared to those of planetary nebulae in different contexts.

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Moonyong Lee,Nguyen Van Duc LongThe “unresolved nuclear region” as Hubble (1926) indicated the bulge of spiral galaxies, became a physically distinct component with the introduction by Baade (1944) of the concept of stellar populations.

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Introduction to the Time Scales Calculus,Without attempting to cover all of the topics discussed at this meeting, I plan to talk briefly about some of the major achievements and ideas that came up here, and then mention a few of the important open questions and some work that might be done to answer them.