The flame ionization detector (FID) has been a commercial analyzer now for about 50 years.
It still finds significant use as a sensitive quantitative monitor of organic compounds in gas …

Comprehensive models of diffuse interstellar clouds - Physical conditions and mo ADS Classic is
now deprecated. It will be completely retired in October 2019. This page will automatically …

Negative ion photoelectron spectroscopyand gas-phase proton transfer kinetics were
employed to determine the CH bond dissociation energies of acetylene, ethylene, and vinyl …

The advent of high-resolution spectrographs and detailed stellar atmosphere modelling has
strengthened the need for accurate molecular data. Carbon-enhanced metal-poor (CEMP) …

All available atomic and molecular signatures of carbon, nitrogen and oxygen are integrated
to provide solar photospheric abundances of the three elements. The CI 8727 wavelength …

The principle objective of this handbook is to provide a readily accessible source of
information on the major fields of spectroscopy. Specifically, these fields are NMR, IR …

Abundances of C and N are derived from features due to the CH G-band and to the UV CN
band measured on high resolution () UVES spectra of more than 40 dwarfs and subgiants in …

Optical absorption line techniques have been applied to the study of a number of translucent
molecular clouds in which the total column densities are large enough that substantial …

The accurate O, Mg and Fe abundances derived in previous papers of this series from a
homogeneous reanalysis of high quality data for a large sample of stars are combined with …

Emission spectroscopy is a 2-D nonintrusive diagnostic technique that offers spatially
resolved data for combustion optimization and control. The UV and visible …