Results 231 to 240 of about 25,554 (268)

Quantifying microbiota impact on plant traits for the guidance of breeding programs

open access: yes
New Phytologist, Volume 250, Issue 6, Page 3524-3533, June 2026.
Manuel Blouin   +5 more
wiley   +1 more source

Extended hot dust emission around the earliest massive quiescent galaxy

open access: yes
Ji Z   +16 more
europepmc   +1 more source

Feedback mechanisms stopping the star formation in a pair of massive galaxies in the early Universe

open access: yes
Pérez-González P   +21 more
europepmc   +1 more source

Star Formation in Irregular Galaxies

Science, 1989
Irregular galaxies can be viewed as laboratories for studying the processes of star formation. This class of galaxy, unlike the more familiar spiral galaxies, forms stars without spiral arms and does so from a chemically less-evolved interstellar medium.
D A, Hunter, J S, Gallagher
openaire   +2 more sources

Star formation in the galaxy

Astrophysics and Space Science, 1972
A previous theory of the authors regarding the planetary system is generalized in an attempt to include star formation. It is found that the theory predicts the correct mass and radius for stellar clusters and also the general shape of the galaxy.
B. W. Pendred, I. P. Williams
openaire   +1 more source

The Evolution of the Star Formation Rate in Galaxies

Astrophysics and Space Science, 2001
The aim of this work is to provide clues for the understanding of the star formation history of the universe. We study the process of star formation in galactic objects in hierarchical clustering scenarios using hydrodynamical cosmological simulations of standard Cold Dark Matter Universe. We estimate the specific star formation rate (sSFR) of galactic
SofÍa Alejandra Cora   +4 more
openaire   +1 more source

Star formation in galaxies

Astronomical & Astrophysical Transactions, 2002
A model of dynamical and chemical evolution of spherical and disk galaxies are discussed. The star formation rate in the model is regulated through ionization of the interstellar hydrogen by massive O,B stars. The volume of a galaxy is determined by the condition of equilibrium between collisional dissipation of turbulent energy of interstellar gas and
openaire   +1 more source

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