Stellar Nucleosynthesis - Astrophysics

Relevant Publications

Measurement of the ^{140}Ce(n,γ) Cross Section at n_TOF and Its Astrophysical Implications for the Chemical Evolution of the Universe.

Issue Release: 2024

Chapter 3: The Origins and Evolution of Planetary Systems.

Issue Release: 2024

One month convection timescale on the surface of a giant evolved star.

Issue Release: 2024

High-temperature Tl decay clarifies Pb dating in early Solar System.

Issue Release: 2024

Search for Na in novae supported by a novel method for measuring femtosecond nuclear lifetimes.

Issue Release: 2023

The 5α condensate state in Ne.

Issue Release: 2023

Measurement of the [Formula: see text]Ta([Formula: see text]) cross sections up to stellar s-process temperatures at the CSNS Back-n.

Issue Release: 2023

Atomic diffusion and mixing in old stars - VIII. Chemical abundance variations in the globular cluster M4 (NGC 6121).

Issue Release: 2023

Collective Neutrino Flavor Instability Requires a Crossing.

Issue Release: 2022

Measurement of F(p, γ)Ne reaction suggests CNO breakout in first stars.

Issue Release: 2022

The Vacuum Cherenkov Detector (VCD) for γ-ray measurements in inertial confinement fusion experiments.

Issue Release: 2022

Imprint of chondrule formation on the K and Rb isotopic compositions of carbonaceous meteorites.

Issue Release: 2021

Electron capture in stars.

Issue Release: 2021

The CO-rich atmosphere of a young accreting super-Jupiter.

Issue Release: 2021

r-Process elements from magnetorotational hypernovae.

Issue Release: 2021

Neutrino Fast Flavor Conversions in Neutron-Star Postmerger Accretion Disks.

Issue Release: 2021

Cluster Analysis of Presolar Silicon Carbide Grains: Evaluation of Their Classification and Astrophysical Implications.

Issue Release: 2021

Direct Measurement of the ^{13}C(α,n)^{16}O Cross Section into the s-Process Gamow Peak.

Issue Release: 2021

3D NLTE spectral line formation of lithium in late-type stars.

Issue Release: 2020

Search for Nova Presolar Grains: γ-Ray Spectroscopy of ^{34}Ar and its Relevance for the Astrophysical ^{33}Cl(p,γ) Reaction.

Issue Release: 2020

What is the Euclid Space Telescope?

What Can Radio Waves Tell Us About the Universe?

What is Bolometric Magnitude?

How Do Nuclear Reactions Power Stars?

Why is Photometry Important in Astrophysics?

What Determines the Position of a Star on the Main Sequence?

How Do We Determine Atmospheric Composition?

How Does Effective Temperature Vary Among Different Types of Stars?

How Has Technology Advanced the Study of Apparent Magnitude?

What is the Cosmic Microwave Background?

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