Titlebook: Stellar Populations; Proceedings of the 1 P. C. Kruit,G. Gilmore Conference proceedings 1995 International Astronomical Union 1995 astronom

Altitude

Stellar Populations in the Magellanic Clouds in metallicities amongst young stars in either Cloud remains tentative. There is no strong evidence for bursts of star formation being triggered by LMC-SMC-Galaxy interactions but the possibility is raised that the SFR in the SMC has been strongly affected by this interaction.

节约

intertwine

Report on the Progress in Stellar Evolution to 1950Dean McLaughlin (1940) gave a review of the current understanding of stellar evolution. At the end he somewhat facetiously remarked that, “..” I would like to suggest that those dates were not chosen randomly, and in the first part of my own survey of stellar evolution to 1950, I would like to expla

stress-response

Spartan

Stellar Evolution and the Population Concept After 1950; The Vatican Conferenceone. Thirteen years after Walter Baade’s seminal papers, the conference reviewed progress in relevant fields of research and formulated a classification of population types that would remain the principal reference for the next decades. I shall review developments preceding the Conference, the initi

熄灭

The Galactic Globular Cluster Systemto distinguish two types of stellar populations, one which is represented by the ordinary H-R diagram (type I), the other by the H-R diagram of the globular clusters (type II). Characteristic of the first type are highly luminous O- and B-type stars and open clusters, of the second, globular cluster

烦躁的女人

glisten

Globular Cluster Systems in Other Galaxies as the paradigmatic Population II objects. Considerable evidence, accumulated especially over the last decade, now demonstrates that globular cluster systems (GCS’s) make up a stellar population with distinctive characteristics of their own and are . just subsets of the old Pop II field stars that

恭维

enumaerate