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Starburst99: Synthesis Models for Galaxies with Active Star Formation
Open accessAbstract
Starburst99 is a comprehensive set of model predictions for spectrophotometric and related properties of galaxies with active star formation. The models are an improved and extended version of the data set previously published by Leitherer & Heckman. We have upgraded our code by implementing the latest set of stellar evolution models of the Geneva group and the model atmosphere grid compiled by Lejeune et al. Several predictions which were not included in the previous publication are shown here for the first time. The models are presented in a homogeneous way for five metallicities between Z = 0.040 and 0.001 and three choices of the initial mass function. The age coverage is 10 6 —10 9 yr. We also show the spectral energy distributions which are used to compute colors and other quantities. The full data set is available for retrieval at a Web site, which allows users to run specific models with nonstandard parameters as well. We also make the source code available to the community.
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“Massive ( ≳ 8 M ⊙ ) stars generate mechanical energy via stellar winds and SNe (Leitherer & Heckman 1995; Leitherer et al. 1999; Sternberg et al. 2003).”
From The Fermi/eROSITA bubbles: a look into the nuclear outflow from the Milky Way (2024) · cites this paper as Leitherer et al. 1999
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Cited by
Sorted by citations
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“The results cited here use the Starburst99 models of Leitherer et al. (1999), which are regularly updated in the on-line version of the package.”
MethodTheoretical Modeling of Starburst Galaxies
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THE STAR FORMATION EFFICIENCY IN NEARBY GALAXIES: MEASURING WHERE GAS FORMS STARS EFFECTIVELY
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Maraston, C. (2005) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2005.09270.x · Cited by 1,907
Metadata
- Authors
- 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.
- Affiliations
- Space Telescope Science Institute (US)
- Observatoire Midi-Pyrénées (FR)
- University of Pennsylvania (US)
- Université Laval (CA)
- Johns Hopkins University (US)
- Venue
- The Astrophysical Journal Supplement Series
- Publisher
- American Astronomical Society
- Published
- 1999-07
- Volume
- 123
- Issue
- 1
- Pages
- 3-40
- ISSN
- 0067-0049 (ISSN-L)
- 1538-4365
- OpenAlex
- W2041127769
- Cited by
- 4,126
- References
- 38
- Citations by year
- 2026: 95 · 2025: 172 · 2024: 166 · 2023: 150 · 2022: 165 · 2021: 160 · 2020: 165 · 2019: 161 · 2018: 189 · 2017: 189 · 2016: 219 · 2015: 182 · 2014: 152 · 2013: 191 · 2012: 174
- FWCI
- 73.67
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- The Astrophysical Journal Supplement Series (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
- arXiv (Cornell University)
- Astrophysics Source Code Library
- Funders
- National Aeronautics and Space Administration (NAS 526555, 526555)
- Space Telescope Science Institute (NAS5- 26555, 5-26555, 26555)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysics and Star Formation Studies
- Keywords
- Starburst99, starburst galaxies, active star formation, spectral energy distribution, stellar evolution models, model atmospheres, initial mass function, metallicity, galaxy age, galaxy color
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