Titlebook: Galaxy Interactions at Low and High Redshift; Proceedings of the 1 J. E. Barnes,D. B. Sanders Conference proceedings 1999 Springer Science+

刺穿

FANG

https://doi.org/10.1007/978-3-031-08801-8We have investigated 4 Shapley constellations (1996, ., ., 40) to define the associated stellar complexes and their properties. From observed star counts and recent spectral classification we derive an age estimate and the upper mass limit of individual stars in these regions.

capsule

Total Mass and Luminosity of Star Forming Regions in the Lmc: the Predicted Infrared Fluxes,We have investigated 4 Shapley constellations (1996, ., ., 40) to define the associated stellar complexes and their properties. From observed star counts and recent spectral classification we derive an age estimate and the upper mass limit of individual stars in these regions.

intimate

Are the Bulge C-Stars Related to the Sagittarius Dwarf Galaxy?,n stars are in that case not metal-rich as previously thought, but they have a metallicity comparable to the LMC, with an age between 0.1–1 Gyr. A significant fraction of the carbon stars still have luminosities fainter than the lower LMC limit of. A similar trend is present among carbon stars found

疏忽

The High-Velocity Clouds: Galactic or Intergalactic?, stellar metal lines. Our distance bracket 4 < . < 11 kpc places Complex A in the Galactic Halo, at 2.5 < . < 7.5 kpc above the plane; a distance similar to Local Group galaxies is excluded. The HI mass implied lies between 0.15 and 1.2 times 10... Our result precludes local origins for this HVC. It

使增至最大

A Near Infrared Survey of the LMC,distributions of RSG, luminous giants and CO line flux are spatially different from each other. This supports the idea that the position of the active star forming region has changed during the past 10. years. The detected sources are cross-identified with the . Point Source Catalog. Sixty-two of 68

畢業(yè)典禮

Common Food Additives and Spices in Thailandn stars are in that case not metal-rich as previously thought, but they have a metallicity comparable to the LMC, with an age between 0.1–1 Gyr. A significant fraction of the carbon stars still have luminosities fainter than the lower LMC limit of. A similar trend is present among carbon stars found

CORE

https://doi.org/10.1007/978-1-4302-3829-4 stellar metal lines. Our distance bracket 4 < . < 11 kpc places Complex A in the Galactic Halo, at 2.5 < . < 7.5 kpc above the plane; a distance similar to Local Group galaxies is excluded. The HI mass implied lies between 0.15 and 1.2 times 10... Our result precludes local origins for this HVC. It

HACK

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