Results 211 to 220 of about 119,560 (250)
Bound star clusters observed in a lensed galaxy 460 Myr after the Big Bang. [PDF]
Adamo A +27 more
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The Progenitor Systems of Classical Novae in M31. [PDF]
Abelson CS +6 more
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Multi-messenger gravitational lensing. [PDF]
Smith GP +40 more
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Extended hot dust emission around the earliest massive quiescent galaxy
Ji Z +16 more
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Feedback mechanisms stopping the star formation in a pair of massive galaxies in the early Universe
Pérez-González P +21 more
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Star Formation in Irregular Galaxies
Science, 1989Irregular 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
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Star formation quenching in massive galaxies
Nature Astronomy, 2018Understanding how and why star formation turns off in massive galaxies is a major challenge for studies of galaxy evolution. Many theoretical explanations have been proposed, but a definitive consensus is yet to be reached.
A. Man, S. Belli
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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
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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, 2001The 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
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