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The first chemical abundance analysis of K giants in the inner Galactic disc
(2010)
Aims. The elemental abundance structure of the Galactic disc has been extensively studied in the solar neighbourhood using long-lived stars such as F and G dwarfs or K and M giants. These are stars whose atmospheres preserve ...
The first chemical abundance analysis of K giants in the inner Galactic disc
(2010)
Aims. The elemental abundance structure of the Galactic disc has been extensively studied in the solar neighbourhood using long-lived stars such as F and G dwarfs or K and M giants. These are stars whose atmospheres preserve ...
The Galactic disc distribution of planetary nebulae with warm dust emission features - I
(BLACKWELL SCIENCE LTD, 2001-02-01)
We investigate the Galactic disc distribution of a sample of planetary nebulae characterized in terms of their mid-infrared spectral features. The total number of Galactic disc PNe with 8-13 mum spectra is brought up to ...
The age-chemical abundance structure of the Galactic disc - II. alpha-dichotomy and thick disc formation
(Oxford University Press, 2020)
We extend our previous work on the age-chemical abundance structure of the Galactic outer disc to the inner disc (4 < r < 8 kpc) based on the SDSS/APOGEE survey. Different from the outer disc, the inner disc stars exhibit ...
Galactic archaeology in the 21st century : unveiling accretion in the MW disc
(Universidad Andrés Bello, 2022)
The evolution of large galaxies such as the Milky Way (MW) in Λ Cold Dark Matter (ΛCDM)
cosmology is driven by interactions with other galaxies. These interactions affect the structure
of the galaxy in long-lasting ways, ...
The first chemical abundance analysis of k giants in the inner galactic disc
(EDP SCIENCES S A, 2010)