Titlebook: Mass-Losing Pulsating Stars and their Circumstellar Matter; Observations and The Y. Nakada,M. Honma,M. Seki Book 2003 Springer Science+Busi

ANTIC

潜移默化

inferno

ARIA

Three Aspects of Red Giant Studies in the Magellanic Cloudsity function carries informations about the star formation rate in the Clouds and it can be mathematically related to their history. Most AGB stars vary their magnitude in a few to several hundred years time; the one epoch DENIS magnitudes for both Large and Small Magellanic Cloud AGB stars outline the same relations as a function of period

CORE

Structure and Evolution of AGB Stars: Current Understandings and Beyondto the formation and early evolution of our galaxy by these studies. Finally, we discuss the importance of non-standard effects in understanding the actual evolution of AGB stars and introduce some recent attempts to reveal their roles in the internal mixing and nucleosynthesis

Obverse

Mass-Losing and Pulsating AGB Stars in the Magellanic Cloudsavailable model grid, and (3) the period-mass loss rate relation for C-rich SMC stars seems to follow that derived for Galactic carbon-rich Miras, suggesting no explicit dependence of mass loss rate on metallicity

affinity

种族被根除

Myosin

Irrepressible

Photometric Properties of Long-Period Variables in the Large Magellanic Cloudtigated. Stars with large amplitudes and high periodicities were distributed on the only one strip amongst multiple structure on the LMC period-luminosity relation. In the CMD, the five strips were located in the order of the period. The stars with characterized light curves were also discussed