Results 11 to 20 of about 86,516 (190)

Understanding the Duration of Solar and Stellar Flares at Various Wavelengths [PDF]

open access: yesAstrophysical Journal, 2023
Recent irradiance measurements from numerous heliophysics and astrophysics missions including Solar Dynamics Observatory (SDO), GOES, Kepler, TESS, Chandra, the X-ray Multi-Mirror Mission, and NICER have provided critical input into understanding the ...
J. Reep, V. Airapetian
semanticscholar   +1 more source

Application of a Magnetic-field-induced Transition in Fe x to Solar and Stellar Coronal Magnetic Field Measurements [PDF]

open access: yesResearch in Astronomy and Astrophysics, 2022
Magnetic fields play a key role in driving a broad range of dynamic phenomena in the atmospheres of the Sun and other stars. Routine and accurate measurements of the magnetic fields at all the atmospheric layers are of critical importance to understand ...
Yajie Chen   +5 more
semanticscholar   +1 more source

Atomic diffusion in solar-like stars with MESA. Comparison with the Montreal/Montpellier and CESTAM stellar evolution codes [PDF]

open access: yesAstronomy & Astrophysics, 2022
Context. The stellar evolution code Modules for Experiments in Stellar Astrophysics (MESA) is public and is widely used by the community. It includes the possibility of taking several non-standard processes such as atomic di ff usion into account. Even if
Bernardo Campilho, M. Deal, D. Bossini
semanticscholar   +1 more source

Stellar population astrophysics (SPA) with the TNG. The chemical content of the red supergiant population in the Perseus complex [PDF]

open access: yesAstronomy & Astrophysics, 2021
Context. The Perseus complex in the outer disk of the Galaxy hosts a number of clusters and associations of young stars. Gaia is providing a detailed characterization of their kinematic structure and evolutionary properties. Aims.
C. Fanelli   +5 more
semanticscholar   +1 more source

Connecting measurements of solar and stellar brightness variations [PDF]

open access: yesAstronomy & Astrophysics, 2020
Context. A comparison of solar and stellar brightness variations is hampered by the difference in spectral passbands that are used in observations, and also by the possible difference in the inclination of the solar and stellar rotation axes from the ...
N.-E. Nèmec   +11 more
semanticscholar   +1 more source

Stromlo Stellar Tracks: Non-solar-scaled Abundances for Massive Stars [PDF]

open access: yes, 2021
We present the Stromlo Stellar Tracks, a set of stellar evolutionary tracks, computed by modifying the Modules for Experiments in Stellar Astrophysics (MESA) 1D stellar evolution package, to fit the Galactic Concordance abundances for hot (T > 8000 K ...
K. Grasha   +3 more
semanticscholar   +1 more source

Constraining stellar and orbital co-evolution through ensemble seismology of solar-like oscillators in binary systems. A census of oscillating red giants and dwarf stars in Gaia DR3 binaries

open access: yesAstronomy & Astrophysics, 2023
Binary systems constitute a valuable astrophysics tool for testing our understanding of stellar structure and evolution. Systems containing at least one oscillating component are interesting in this regard because asteroseismology offers independent ...
P. G. Beck   +25 more
semanticscholar   +1 more source

Solar System Science with the Orbiting Astronomical Satellite Investigating Stellar Systems (OASIS) Observatory

open access: yesSpace Science Reviews, 2022
The overarching theme of the Orbiting Astronomical Satellite for Investigating Stellar Systems (OASIS), an Astrophysics MIDEX-class mission concept, is Following water from galaxies, through protostellar systems, to Earth’s oceans.
C. Anderson   +8 more
semanticscholar   +1 more source

Stellar Population Astrophysics (SPA) with TNG [PDF]

open access: yesAstronomy & Astrophysics, 2020
Context. Open clusters are excellent tracers of the chemical evolution of the Galactic disc. The spatial distribution of their elemental abundances, through the analysis of high-quality and high-resolution spectra, provides insight into the chemical ...
G. Casali   +11 more
semanticscholar   +1 more source

Stellar population astrophysics (SPA) with the TNG [PDF]

open access: yesAstronomy & Astrophysics, 2019
Context. Open clusters exquisitely track the Galactic disc chemical properties and its time evolution; a substantial number of studies and large spectroscopic surveys focus mostly on the chemical content of relatively old clusters (age ≳ 1 Gyr ...
V. d'orazi   +10 more
semanticscholar   +3 more sources

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