Results 111 to 120 of about 50,982 (241)
The observed chemical diversity of Milky Way stars places important constraints on Galactic chemical evolution and the mixing processes that operate within the interstellar medium. Recent works have found that the chemical diversity of disk stars is low.
Catherine Manea +5 more
doaj +1 more source
A metal-poor star with abundances from a pair-instability supernova. [PDF]
Xing QF +9 more
europepmc +1 more source
Abundances in galactic H2 regions, 3: G25.4-0.2, G45.5+0.06, M8, S159 and DR22 [PDF]
Measurements of the ARII (6.99 microns), ArIII (8.99 microns), NeII (12.81 microns), SIII (18.71 microns), and SIV (10.51 microns) lines are presented for five compact HII regions along with continuum spectroscopy.
Briotta, D. A., Jr. +6 more
core +1 more source
Investigating Phosphorus Abundances in a Sample of APOGEE-2 Bulge Globular Clusters
Phosphorus-enhanced (P-rich; [P/Fe] ≳ +0.8) giants have been found among mildly metal-poor field stars, but in only one star in a globular cluster (GC), M4 (NGC 6121).
Beatriz Barbuy +11 more
doaj +1 more source
Whither or Wither the Sulfur Anomaly in Planetary Nebulae?
We present a thorough investigation of the long-standing sulfur anomaly enigma. Our analysis uses chemical abundances from the most extensive data set available for 126 planetary nebulae (PNs) with improved accuracy and reduced uncertainties from a 10° ×
Shuyu Tan, Quentin A. Parker
doaj +1 more source
The age of the galactic cosmic rays derived from the abundance of Be-10
M. García-Muñoz +2 more
openalex +1 more source
The Deuterium Abundance In The Galactic Center 50 km/s Molecular Cloud: Evidence For A Cosmological Origin Of D [PDF]
D. A. Lubowich +6 more
openalex +1 more source
Revealing the Origins of Galactic Globular Clusters via their Mg–Al Abundances
Many Galactic globular clusters (GCs) originated in diverse host galaxies before being subsequently incorporated into the Milky Way through hierarchical galaxy assembly. Identifying their origins is crucial for revealing galaxy properties at early times.
Shihui Lin +6 more
doaj +1 more source
A secondary tracer approach to the derivation of galactic cosmic-ray source isotopic abundances
E. C. Stone, M. E. Wiedenbeck
openalex +1 more source
Using Cepheids to determine the galactic abundance gradient [PDF]
S. M. Andrievsky +6 more
openalex +3 more sources

