The first CEMP-no star in the Sculptor dwarf spheroidal galaxy
Aula GrattonThe origin of carbon-enhanced metal-poor (CEMP) stars and their possible connection with the chemical elements
The origin of carbon-enhanced metal-poor (CEMP) stars and their possible connection with the chemical elements
The origin of carbon-enhanced metal-poor (CEMP) stars and their possible connection with the chemical elements
Coevolutionary models that link the growth of supermassive black holes (BHs) and of their host
Coevolutionary models that link the growth of supermassive black holes (BHs) and of their host
Six Large Magellanic Cloud (LMC) globular clusters (GCs) (NGC 1466, NGC 1841, NGC 2210, NGC
Six Large Magellanic Cloud (LMC) globular clusters (GCs) (NGC 1466, NGC 1841, NGC 2210, NGC
I present observations of dynamic, slender bright fibrils seen in high-quality narrow-band Ca II H
I present observations of dynamic, slender bright fibrils seen in high-quality narrow-band Ca II H
In the standard cosmological model ninety-five percent of the energy content of the universe consists
In the standard cosmological model ninety-five percent of the energy content of the universe consists
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