The DOI matches its Crossref record; 2 of the 2 references it cites were found in a registry or an index.
Properties of planets in binary systems: The role of binary separation
Open accessAbstract
Aims.The statistical properties of planets in binaries were investigated. Any difference to planets orbiting single stars can shed light on the formation and evolution of planetary systems. As planets were found around components of binaries with very different separation and mass ratio, it is particularly important to study the characteristics of planets as a function of the effective gravitational influence of the companion.
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Butler, R. P., Wright, J. T., Marcy, G. W., Fischer, D. A., Vogt, S. S., Tinney, C. G., Jones, H. R. A., Carter, B. D., Johnson, J. A., McCarthy, C., et al. (2006) · The Astrophysical Journal · doi:10.1086/504701 · Cited by 914
Relative velocities among accreting planetesimals in binary systems: The circumprimary case
THEBAULT, P., MARZARI, F., & SCHOLL, H. (2006) · Icarus · doi:10.1016/j.icarus.2006.01.022 · Cited by 145
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Metadata
- Authors
- Desidera, S., & Barbieri, M.
- Venue
- Astronomy & Astrophysics
- Publisher
- EDP Sciences
- Published
- 2006-10-24
- Volume
- 462
- Issue
- 1
- Pages
- 345-353
- ISSN
- 0004-6361 (ISSN-L)
- 1432-0746
- OpenAlex
- W4298858430
- Cited by
- 209
- References
- 2
- FWCI
- 9.45
- Type
- journal article
- Language
- en
- Open access
- bronze
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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.