Results 181 to 190 of about 14,525 (205)

Transient colonization by Priestia megaterium B1L5 alters the structure of the rhizosphere microbiome towards potential plant beneficial bacterial groups in apple plantlets. [PDF]

Environ Microbiome
Mahmoud FM, Edelmann H, Si Y, Endrejat L, Pritsch K, Gutjahr C, Ehrenreich A, Winkelmann T, Winkler JB, Schnitzler JP, Schloter M.   +10 more
europepmc   +1 more source

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Star formation quenching in galaxies

EAS Publications Series, 2012
We investigate the correlation of star formation quenching with internal galaxy properties and environment by comparing observation and theoretical models. We first classify galaxies as the most massive "central" or "satellite" in each halo in order to investigate the environmental effect.
T. Kimm, R. S. Somerville, S. K. Yi, van den Bosch F. C., S. Salim, F. Fontonot, MONACO, Pierluigi, H. J. Mo, A. Pasquali, R. M. Rich, X. Yang   +10 more
openaire   +2 more sources

The epoch of galaxy quenching

Nature Astronomy, 2023
Emma Curtis-Lake, Asa Bluck, Francesco d’Eugenio, Roberto Maiolino, Debora Sijacki   +4 more
openaire   +1 more source

The Role of Galaxy Environment in Quenching Galaxy Star Formation

2017
How galaxies transition between blue, star-forming, spirals and red elliptical galaxies is a key question in modern extragalactic astrophysics. Galaxies will transition between the two broad populations under competing influences including internal structure, gravitational interactions, black hole feedback, and group and cluster environment.
openaire   +1 more source

A repeating fast radio burst source localized to a nearby spiral galaxy

Nature, 2020
Benito Marcote, Kenzie Nimmo, Jason Hessels   +2 more
exaly  

Cosmological simulations of galaxy formation

Nature Reviews Physics, 2020
Mark Vogelsberger, Federico Marinacci, Paul Torrey   +2 more
exaly  

The Quenching of Cluster Galaxies

In this thesis we present two projects investigating the evolution and quenching of cluster galaxy star formation (SF) activity. Leveraging a sample of 36 galaxy clusters, we measure the level of member SF activity. Over the 7.5 billion years spanned by our clusters, from z=1.5 to z=0.15, the SF activity of cluster galaxies decreases by a factor of 11.
openaire   +1 more source

Evidence for neutrino emission from the nearby active galaxy NGC 1068

Science, 2022
exaly  

The Galaxy in Context: Structural, Kinematic, and Integrated Properties

Annual Review of Astronomy and Astrophysics, 2016
Joss Bland-Hawthorn, Ortwin Gerhard
exaly  

Physical Models of Galaxy Formation in a Cosmological Framework

Annual Review of Astronomy and Astrophysics, 2015
Romeel Dave
exaly