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Cited by 730

The DOI matches its Crossref record; 1 of the 1 references it cites were found in a registry or an index.

High-Energy Processes in Young Stellar Objects

Feigelson, Eric D., Montmerle, Thierry·1999·Annual Review of Astronomy and Astrophysics

Abstract

▪ Abstract Observational studies of low-mass stars during their early stages of evolution, from protostars through the zero-age main sequence, show highly elevated levels of magnetic activity. This activity includes strong fields covering much of the stellar surface and powerful magnetic reconnection flares seen in the X-ray and radio bands. The flaring may occur in the stellar magnetosphere, at the star-disk interface, or above the circumstellar disk. Ionization from the resulting high-energy radiation may have important effects on the astrophysics of the disk, such as promotion of accretion and coupling to outflows, and on the surrounding interstellar medium. The bombardment of solids in the solar nebula by flare shocks and energetic particles may account for various properties of meteorites, such as chondrule melting and spallogenic isotopes. X-ray surveys also improve our samples of young stars, particularly in the weak-lined T Tauri phase after disks have dissipated, with implications for our understanding of star formation in the solar neighborhood.

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Crossref · 10.1146/annurev.astro.37.1.363

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Metadata

Authors
Feigelson, E. D., & Montmerle, T.
Venue
Annual Review of Astronomy and Astrophysics
Published
1999-09
Volume
37
Issue
1
Pages
363-408
ISSN
  • 0066-4146 (ISSN-L)
  • 1545-4282
OpenAlex
W2166931875
Cited by
730
References
1
FWCI
3.66
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: High-Energy Processes in Young Stellar Objects. https://app.cochat.ai/papers/10.1146/annurev.astro.37.1.363
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Feigelson, E. D., & Montmerle, T. (1999). High-Energy Processes in Young Stellar Objects. Annual Review of Astronomy and Astrophysics. https://doi.org/10.1146/annurev.astro.37.1.363

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

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