Results 41 to 50 of about 5,073 (240)

Prospects for asteroseismology [PDF]

open access: yesAstrophysics and Space Science, 2009
Proc. HELAS Workshop on 'Synergies between solar and stellar modelling', eds M. Marconi, D. Cardini & M. P. Di Mauro, Astrophys.
Christensen-Dalsgaard, Jørgen   +1 more
openaire   +5 more sources

Magnetic and Rotational Evolution of ρ CrB from Asteroseismology with TESS [PDF]

open access: yesAstrophysical Journal, 2021
During the first half of main-sequence lifetimes, the evolution of rotation and magnetic activity in solar-type stars appears to be strongly coupled. Recent observations suggest that rotation rates evolve much more slowly beyond middle age, while stellar
T. Metcalfe   +17 more
semanticscholar   +1 more source

Detection and Optimization of Traffic Networks Based on Voronoi Diagram

open access: yesDiscrete Dynamics in Nature and Society, Volume 2021, Issue 1, 2021., 2021
Traffic peak is an important parameter of modern transport systems. It can be used to calculate the indices of road congestion, which has become a common problem worldwide. With accurate information about traffic peaks, transportation administrators can make better decisions to optimize the traffic networks and therefore enhance the performance of ...
Rui Tao   +6 more
wiley   +1 more source

Asteroseismology Across the Hertzsprung–Russell Diagram

open access: yesAnnual Review of Astronomy and Astrophysics, 2022
Asteroseismology has grown from its beginnings three decades ago to a mature field teeming with discoveries and applications. This phenomenal growth has been enabled by space photometry with precision 10–100 times better than ground-based observations ...
D. Kurtz
semanticscholar   +1 more source

The Pre-main Sequence: Challenges and Prospects for Asteroseismology

open access: yesFrontiers in Astronomy and Space Sciences, 2022
Stars do not simply pop up on the main sequence. Before the stars arrive on the zero-age main sequence, they form in the collapses of molecular clouds, gain matter through accretion processes, and compress their cores until hydrogen can burn in full ...
Konstanze Zwintz, Thomas Steindl
doaj   +1 more source

A Need to Revise Stellar Opacities from Asteroseismology of δ Scuti Stars [PDF]

open access: yesAstrophysical Journal Letters, 2022
We construct seismic models of the four double-mode radial δ Scuti stars adopting opacities from three databases: OPAL, OP, and OPLIB. The aim is to find the models that fit the observed frequencies of the two radial modes and have the effective ...
J. Daszyńska-Daszkiewicz   +4 more
semanticscholar   +1 more source

On the Detectability of Large-Scale Flows by Asteroseismology

open access: yesFrontiers in Astronomy and Space Sciences, 2020
Large-scale convective motions are an integral part of stellar interior dynamics and might play a relevant role in stellar dynamo processes. However, they are difficult to detect or characterize.
Markus Roth, Wiebke Herzberg
doaj   +1 more source

CubeSpec space mission. I. Asteroseismology of massive stars from time series optical spectroscopy: science requirements and target list prioritisation [PDF]

open access: yesAstronomy & Astrophysics, 2021
Context. There is currently a niche for providing high-cadence, high resolution, time-series optical spectroscopy from space, which can be filled by using a low-cost cubesat mission.
D. Bowman   +10 more
semanticscholar   +1 more source

A review on Asteroseismology [PDF]

open access: yesProceedings of Frontier Research in Astrophysics – II — PoS(FRAPWS2016), 2017
Over the last decade, thanks to the successful space missions launched to detect stellar pulsations, Asteroseismology has produced an extraordinary revolution in astrophysics, unveiling a wealth of results on structural properties of stars over a large part of the H-R diagram.
Maria Pia, di Mauro
openaire   +4 more sources

White Dwarfs as Physics Laboratories: Lights and Shadows

open access: yesFrontiers in Astronomy and Space Sciences, 2022
The evolution of white dwarfs is essentially a gravothermal process of cooling in which the basic ingredients for predicting their evolution are well identified, although not always well understood. There are two independent ways to test the cooling rate.
J. Isern   +6 more
doaj   +1 more source

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