Results 91 to 100 of about 50,982 (241)
Boo-1137 - An Extremely Metal-Poor Star in the Ultra-Faint Dwarf Spheroidal Galaxy Bo\"{o}tes I
We present high-resolution, high-S/N spectra of an extremely metal- poor giant star Boo-1137 in the "ultra-faint" dwarf spheroidal galaxy (dSph) Bootes I (absolute magnitude Mv ~ -6.3).
Abazajian +35 more
core +1 more source
PN Abundances in Different Galactic Systems [PDF]
Developments in the measurement of abundances in planetary nebulae since IAU Symposium 131 are reviewed. Present uncertainties and outstanding problems in the interpretation of emission-line measurements are discussed. Results for different samples of PN are reviewed, in terms of the galactic site.
openaire +2 more sources
CHEMICAL COMPOSITION OF ATMOSPHERES OF COOL GIANT STARS
Results of determination of abundances of chemical elements in the atmospheres of 57 giant stars of the oxygen sequence of the Galactic disk axe given.
N. S. Komarov
doaj +1 more source
On the Abundance of Heavy Elements in the Galactic Centre [PDF]
D. K. Aitken +2 more
openalex +1 more source
Chemical Abundances of Planetary Nebulae in M33
Using spectroscopic data presented in Magrini et al. (2003), we have analyzed with the photoionization code CLOUDY 94.00 (Ferland et al. 1998) 11 Planetary Nebulae belonging to the spiral galaxy M 33. Central star temperatures and nebular parameters have
A. Mampaso +33 more
core +1 more source
MOLYBDENUM AND RUTHENIUM IN THE GALAXY
We present a brief overview of the molybdenum and ruthenium present-day nucleosynthesis calculations and abundance determinations in stars belonging to different substructures (populations) in the Galaxy.
T. V. Mishenina, T. I. Gorbaneva
doaj +1 more source
The galactic abundance gradient [PDF]
Lynette M. Newton +4 more
openaire +2 more sources
Elemental abundances in the centre of the Galactic nuclear disc
ABSTRACT We have made the first attempt to derive the chemical properties of the Galactic disc at its very central part using high-resolution infrared spectroscopic observations of four classical Cepheids. These stars are located at Galactocentric distances smaller than 1 kpc.
Walter J. Maciel +10 more
openaire +5 more sources
Phosphorus-bearing molecules PO and PN at the edge of the Galaxy. [PDF]
Koelemay LA, Gold KR, Ziurys LM.
europepmc +1 more source

