Results 341 to 350 of about 4,372,191 (364)

Small Molecules as Markers for Decoding Plastic-Related Information: A Focus on Polymer Composition. [PDF]

Environ Sci Technol Lett
Li Y, Poisson K, McMinn MH, Zhang C, Yang S, Tian Z.   +5 more
europepmc   +1 more source

Tracing chemical depletion in evolved binaries hosting second-generation transition discs. [PDF]

Mon Not R Astron Soc
Mohorian M, Kamath D, Menon M, Amarsi AM, Van Winckel H, Fava C, Andrych K.   +6 more
europepmc   +1 more source

Enrichment of moderately volatile elements in first-generation planetesimals of the inner Solar System. [PDF]

Sci Adv
Grewal DS, Bhattacharjee S, Zhang B, Nie NX, Miyazaki Y.   +4 more
europepmc   +1 more source

Microbial communities in glacial lakes of Glacier National Park, MT, USA. [PDF]

FEMS Microbiol Ecol
Peoples LM, Giersch JJ, Tappenbeck TH, Vanderwall JW, Ranieri JM, Vick-Majors TJ, Elser JJ, Church MJ.   +7 more
europepmc   +1 more source

Chemical abundances of planet-host stars. Results for alpha and Fe-group elements

, 2003
A. Bodaghee, N. C. Santos, G. Israelian, M. Mayor   +3 more
openalex  

Some of the next articles are maybe not open access.

Related searches:

Chemical abundances in high-redshift galaxies: a powerful new emission line diagnostic

, 2016
This Letter presents a new, remarkably simple diagnostic specifically designed to derive chemical abundances for high redshift galaxies. It uses only the Hα$\mathrm{H}\alpha$, [N ii] and [S ii] emission lines, which can usually be observed in a single ...
M. Dopita, L. Kewley, R. Sutherland, D. Nicholls   +3 more
semanticscholar   +1 more source

Chemical Abundances of Symbiotic Giants [PDF]

EAS Publications Series, 2015
High resolution (R ∼ 50000), near-IR spectra were used to measure photospheric abundances of CNO and elements around the iron peak for 24 symbiotic giants. Spectrum synthesis was employed using local thermal equilibrium and hydrostatic model atmospheres. The metallicities are distributed in a wide range with maximum around [ Fe / H ] ∼−0.4 – − 0.3 dex.
J. Mikolajewska, R.R. Joyce, K.H. Hinkle, C. Galan   +3 more
openaire   +1 more source