Results 261 to 270 of about 197,808 (272)

Data Report: Educational pathway addressing food and nutrition in amyotrophic lateral sclerosis on the AVASUS platform. [PDF]

open access: yesFront Digit Health
Coutinho KMD   +7 more
europepmc   +1 more source

A population of faint, old, and massive quiescent galaxies at [Formula: see text] revealed by JWST NIRSpec Spectroscopy. [PDF]

open access: yesSci Rep
Nanayakkara T   +15 more
europepmc   +1 more source

QnAs with Katherine Freese. [PDF]

open access: yesProc Natl Acad Sci U S A
Gabrielsen P.
europepmc   +1 more source

Understanding the Formation of Saturn's Regular Moons in the Context of Giant Planet Moons Formation Scenarios. [PDF]

open access: yesSpace Sci Rev
Blanc M   +9 more
europepmc   +1 more source

An Abrupt Change in the Disk Fraction of Free-Floating Planets at the Deuterium-Burning Ignition Limit

open access: yes
Rodrigues T   +11 more
europepmc   +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

Massive stars in the UV [PDF]

open access: possibleAstrophysics and Space Science, 2006
We emphasize in this paper the importance of the UV range for our knowledge of massive stars and the fundamental role played by past and present space-based UV capabilities (IUE, HST, FUSE and others). Based on a review of the work developed in the last years and the state of the art situation for quantitative spectroscopy of massive stars, we present ...
Francisco Najarro   +2 more
openaire   +1 more source

Nucleosynthesis in Massive Stars

Space Science Reviews, 1993
We discuss three aspects of the nucleosynthesis in massive and intermediate—mass stars during their early evolutionary phases. These are related to the CNO abundances in giant or supergiant stars, to the 26A1 yield from massive stars via stellar wind, and to the production of the s—process nuclei in massive stars.
openaire   +2 more sources

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