Results 291 to 300 of about 948,048 (332)

Consumption of traditional Sardinian fermented milk promotes changes in the rat gut microbiota composition and functions. [PDF]

open access: yesBMC Microbiol
Abbondio M   +10 more
europepmc   +1 more source

Primordial Rotating Disk Composed of ≥15 Star Forming Clumps at Cosmic Dawn

open access: yes
Fujimoto S   +45 more
europepmc   +1 more source

lefser: implementation of metagenomic biomarker discovery tool, LEfSe, in R. [PDF]

open access: yesBioinformatics
Khleborodova A   +5 more
europepmc   +1 more source

Selective recruitment of beneficial microbes in the rhizosphere of maize affected by microbial inoculants, farming practice, and seasonal variations. [PDF]

open access: yesEnviron Microbiome
Kampouris ID   +13 more
europepmc   +1 more source

A Non-Metaproteomics Researchers' View on Metaproteomics in Microbiome Research. [PDF]

open access: yesProteomics
Aho VTE   +5 more
europepmc   +1 more source

Abundances in Galaxies

Astrophysics and Space Science, 2001
To start things going, the following topics were suggested:* 1. Reliability of abundances Stars vs H ii regions H ii classical diagnostics Effects of shocks and inhomogeneities on H ii-region diagnostics H n new diagnostics Can reliable H ii-region diagnostics be developed for high metallicity?
B. E. J. Pagel, M. G. Edmunds
openaire   +1 more source

Abundances in dwarf galaxies

AIP Conference Proceedings, 1989
In an attempt to discover regions of very low heavy element abundance, we have observed H II regions in 7 nearby, very low luminosity dwarf irregular galaxies. All yield oxygen abundances of less than one‐tenth of the solar value, and three are within a factor of two of the lowest oxygen abundance ever detected in an H II region.
Evan D. Skillman, R. C. Kennicutt
openaire   +1 more source

The evolution of abundances in the galaxy

AIP Conference Proceedings, 1989
This very brief review of the evolution of the abundances in our Galaxy first recalls the main observational facts regarding such abundances which have to be taken into account by any model of chemical evolution of our Galaxy. After having defined what are the crucial parameters which define such models, the emphasis is made on two approaches: the ...
openaire   +1 more source

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