The DOI matches its Crossref record; 2 of the 2 references it cites were found in a registry or an index.
The metal-rich nature of stars with planets
Open accessAbstract
With the goal of confirming the metallicity "excess" present in stars with planetary-mass companions, we present in this paper a high-precision spectroscopic study of a sample of dwarfs included in the CORALIE extrasolar planet survey. The targets were chosen according to the basic criteria that 1) they formed part of a limited volume and 2) they did not present the signature of a planetary host companion. A few stars with planets were also observed and analysed; namely, HD 6434, HD 13445 (Gl 86), HD 16141, HD 17051 (ι Hor), HD 19994, HD 22049 (ϵ Eri), HD 28185, HD 38529, HD 52265, HD 190228, HD 210277 and HD 217107. For some of these objects there had been no previous spectroscopic studies. The spectroscopic analysis was done using the same technique as in previous work on the metallicity of stars with planets, thereby permitting a direct comparison of the results. The work described in this paper thus represents the first uniform and unbiased comparison between stars with and without planetary-mass companions in a volume-limited sample. The results show that 1) stars with planets are significantly metal-rich, and 2) that the source of the metallicity is most probably "primordial" . The results presented here may impose serious constraints on planetary system formation and evolution models.
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Cites
A Jupiter-mass companion to a solar-type star
Mayor, M., & Queloz, D. (1995) · Nature · doi:10.1038/378355a0 · Cited by 4,111
Self-citationOrbital migration of the planetary companion of 51 Pegasi to its present location
Lin, D. N. C., Bodenheimer, P., & Richardson, D. C. (1996) · Nature · doi:10.1038/380606a0 · Cited by 1,235
Cited by
Dawson, R. I., & Johnson, J. A. (2018) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081817-051853 · Cited by 622
High‐Resolution Submillimeter Constraints on Circumstellar Disk Structure
Andrews, S. M., & Williams, J. P. (2007) · The Astrophysical Journal · doi:10.1086/511741 · Cited by 426
Tidal Dissipation in Rotating Giant Planets
Ogilvie, G. I., & Lin, D. N. C. (2004) · The Astrophysical Journal · doi:10.1086/421454 · Cited by 386
THE FREQUENCY OF HOT JUPITERS ORBITING NEARBY SOLAR-TYPE STARS
Wright, J. T., Marcy, G. W., Howard, A. W., Johnson, J. A., Morton, T. D., & Fischer, D. A. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/753/2/160 · Cited by 371
THE COMPOSITIONAL DIVERSITY OF EXTRASOLAR TERRESTRIAL PLANETS. I. IN SITU SIMULATIONS
Bond, J. C., O'Brien, D. P., & Lauretta, D. S. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/715/2/1050 · Cited by 308
Metadata
- Authors
- Santos, N. C., Israelian, G., & Mayor, M.
- Venue
- Astronomy & Astrophysics
- Publisher
- EDP Sciences
- Published
- 2001-07
- Volume
- 373
- Issue
- 3
- Pages
- 1019-1031
- ISSN
- 0004-6361 (ISSN-L)
- 1432-0746
- OpenAlex
- W2078699511
- Cited by
- 477
- References
- 2
- FWCI
- 19.75
- Type
- journal article
- Language
- en
- Open access
- bronze
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- Santos, N. C., Israelian, G., & Mayor, M. (2001). The metal-rich nature of stars with planets. Astronomy & Astrophysics. https://doi.org/10.1051/0004-6361%3A20010648
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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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