The DOI matches its Crossref record; 1 of the 1 references it cites were found in a registry or an index.
Winds from Hot Stars
Abstract
▪ Abstract This review deals with the winds from “normal” hot stars such as O-stars, B- and A-supergiants, and Central Stars of Planetary Nebulae with O-type spectra. The advanced diagnostic methods of stellar winds, including an assessment of the accuracy of the determinations of global stellar wind parameters (terminal velocities, mass-loss rates, wind momenta, and energies), are introduced and scaling relations as a function of stellar parameters are provided. Observational results are interpreted in the framework of the stationary, one-dimensional (1-D) theory of line-driven winds. Systematic effects caused by nonhomogeneous structures, time dependence, and deviations from spherical symmetry are discussed. The review finishes with a brief description of the role of stellar winds as extragalactic distance indicators and as tracers of the chemical composition of galaxies at high redshift.
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Citations
Cites
Starburst99: Synthesis Models for Galaxies with Active Star Formation
Leitherer, C., Schaerer, D., Goldader, J. D., Delgado, R. M. G., Robert, C., Kune, D. F., de Mello, D. F., Devost, D., & Heckman, T. M. (1999) · The Astrophysical Journal Supplement Series · doi:10.1086/313233 · Cited by 4,126
Cited by
Binary Interaction Dominates the Evolution of Massive Stars
Sana, H., de Mink, S. E., de Koter, A., Langer, N., Evans, C. J., Gieles, M., Gosset, E., Izzard, R. G., Le Bouquin, J.-B., & Schneider, F. R. N. (2012) · Science · doi:10.1126/science.1223344 · Cited by 2,118
The Initial Mass Function of Stars: Evidence for Uniformity in Variable Systems
Kroupa, P. (2002) · Science · doi:10.1126/science.1067524 · Cited by 1,793
A new calibration of stellar parameters of Galactic O stars
Martins, F., Schaerer, D., & Hillier, D. J. (2005) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20042386 · Cited by 1,120
Mass Loss: Its Effect on the Evolution and Fate of High-Mass Stars
Smith, N. (2014) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081913-040025 · Cited by 1,042
“A previous review by Kudritzki & Puls (2000) (KP00 hereafter) dealt with line-driven winds of hot stars, focussing on the theory of the driving mechanism as well as common scaling relations used to convert observables to rates.”
BackgroundAbbott, B. P., Abbott, R., Abbott, T. D., Abraham, S., Acernese, F., Ackley, K., Adams, C., Adhikari, R. X., Adya, V. B., Affeldt, C., et al. (2019) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/ab3800 · Cited by 895
Metadata
- Authors
- Kudritzki, R.-P., & Puls, J.
- Venue
- Annual Review of Astronomy and Astrophysics
- Publisher
- Annual Reviews
- Published
- 2000-09
- Volume
- 38
- Issue
- 1
- Pages
- 613-666
- ISSN
- 0066-4146 (ISSN-L)
- 1545-4282
- OpenAlex
- W2123423036
- Cited by
- 771
- References
- 1
- FWCI
- 2.38
- Type
- journal article
- Language
- en
- Open access
- closed
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- Kudritzki, R.-P., & Puls, J. (2000). Winds from Hot Stars. Annual Review of Astronomy and Astrophysics. https://doi.org/10.1146/annurev.astro.38.1.613
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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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