The DOI matches its Crossref record; 113 of the 113 references it cites were found in a registry or an index.
Young Stars Near the Sun
Abstract
▪ Abstract Until the late 1990s the rich Hyades and the sparse UMa clusters were the only coeval, comoving concentrations of stars known within 60 pc of Earth. Both are hundreds of millions of years old. Then beginning in the late 1990s the TW Hydrae Association, the Tucana/Horologium Association, the β Pictoris Moving Group, and the AB Doradus Moving Group were identified within ∼60 pc of Earth, and the η Chamaeleontis cluster was found at 97 pc. These young groups (ages 8–50 Myr), along with other nearby, young stars, will enable imaging and spectroscopic studies of the origin and early evolution of planetary systems.
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Citations
Cites
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Pre-Main-Sequence Evolution in the Taurus-Auriga Molecular Cloud
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Disk frequencies and lifetimes in Young clusters
Haisch, Jr., Lada, E. A., & Lada, C. J. (2001) · The Astrophysical Journal · doi:10.1086/320685 · Cited by 1,723
A [ITAL]Hipparcos[/ITAL] Census of the Nearby OB Associations
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Dynamics of binary-disk interaction. 1: Resonances and disk gap sizes
Artymowicz, P., & Lubow, S. H. (1994) · The Astrophysical Journal · doi:10.1086/173679 · Cited by 1,317
Disk Frequencies and Lifetimes in Young Clusters
Haisch, K. E., & Lada, C. J. (2001) · CERN Document Server (European Organization for Nuclear Research) · Cited by 1,074
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A Circumstellar Disk Around β Pictoris
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High-Energy Processes in Young Stellar Objects
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The SuperCOSMOS Sky Survey - I. Introduction and description
Hambly, N. C., MacGillivray, H. T., Read, M. A., Tritton, S. B., Thomson, E. B., Kelly, B. D., Morgan, D. H., Smith, R. E., Driver, S. P., Williamson, J., et al. (2001) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2001.04660.x · Cited by 621
Cited by
INTRINSIC COLORS, TEMPERATURES, AND BOLOMETRIC CORRECTIONS OF PRE-MAIN-SEQUENCE STARS
Pecaut, M. J., & Mamajek, E. E. (2013) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/208/1/9 · Cited by 2,407
Improved Age Estimation for Solar‐Type Dwarfs Using Activity‐Rotation Diagnostics
Mamajek, E. E., & Hillenbrand, L. A. (2008) · The Astrophysical Journal · doi:10.1086/591785 · Cited by 1,313
Wyatt, M. C. (2008) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.45.051806.110525 · Cited by 936
Search for associations containing young stars (SACY): I. Sample and searching method
Torres, C. A. O., Quast, G. R., da Silva, L., de la Reza, R., Melo, C. H. F., & Sterzik, M. (2006) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20065602 · Cited by 632
The SkyMapper Telescope and The Southern Sky Survey
Keller, S. C., Schmidt, B. P., Bessell, M. S., Conroy, P. G., Francis, P., Granlund, A., Kowald, E., Oates, A. P., Martin-Jones, T., Preston, T., et al. (2007) · Publications of the Astronomical Society of Australia · doi:10.1071/as07001 · Cited by 538
Metadata
- Authors
- Zuckerman, B., & Song, I.
- Venue
- Annual Review of Astronomy and Astrophysics
- Publisher
- Annual Reviews
- Published
- 2004-09-22
- Volume
- 42
- Issue
- 1
- Pages
- 685-721
- ISSN
- 0066-4146 (ISSN-L)
- 1545-4282
- OpenAlex
- W2126530770
- Cited by
- 594
- References
- 113
- FWCI
- 2.56
- Type
- journal article
- Language
- en
- Open access
- closed
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.
