The DOI matches its Crossref record; 9 of the 9 references it cites were found in a registry or an index.
The Occurrence and Architecture of Exoplanetary Systems
Open accessAbstract
The basic geometry of the Solar System—the shapes, spacings, and orientations of the planetary orbits—has long been a subject of fascination as well as inspiration for planet-formation theories. For exoplanetary systems, those same properties have only recently come into focus. Here we review our current knowledge of the occurrence of planets around other stars, their orbital distances and eccentricities, the orbital spacings and mutual inclinations in multiplanet systems, the orientation of the host star's rotation axis, and the properties of planets in binary-star systems.
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Citations
Cites
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Giant Planet Formation by Gravitational Instability
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“The only other theory that is occasionally discussed is gravitational instability, in which the gaseous disk collapses directly into giant planets (Boss 1997).”
BackgroundGiant Planet Occurrence in the Stellar Mass-Metallicity Plane
Johnson, J. A., Aller, K. M., Howard, A. W., & Crepp, J. R. (2010) · Publications of the Astronomical Society of the Pacific · doi:10.1086/655775 · Cited by 782
HOT STARS WITH HOT JUPITERS HAVE HIGH OBLIQUITIES
Winn, J. N., Fabrycky, D., Albrecht, S., & Johnson, J. A. (2010) · The Astrophysical Journal · doi:10.1088/2041-8205/718/2/l145 · Cited by 735
Self-citationOBLIQUITIES OF HOT JUPITER HOST STARS: EVIDENCE FOR TIDAL INTERACTIONS AND PRIMORDIAL MISALIGNMENTS
Albrecht, S., Winn, J. N., Johnson, J. A., Howard, A. W., Marcy, G. W., Butler, R. P., Arriagada, P., Crane, J. D., Shectman, S. A., Thompson, I. B., et al. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/757/1/18 · Cited by 664
Self-citationThe Occurrence and Mass Distribution of Close-in Super-Earths, Neptunes, and Jupiters
Howard, A. W., Marcy, G. W., Johnson, J. A., Fischer, D. A., Wright, J. T., Isaacson, H., Valenti, J. A., Anderson, J., Lin, D. N. C., & Ida, S. (2010) · Science · doi:10.1126/science.1194854 · Cited by 635
One or more bound planets per Milky Way star from microlensing observations
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THE FREQUENCY OF HOT JUPITERS ORBITING NEARBY SOLAR-TYPE STARS
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“The discrepancy might be attributable to differences in metallicity or the frequency of multiple-star systems between the two samples (Gould et al. 2006, Bayliss & Sackett 2011, Wright et al. 2012).”
Background
Cited by
Ngo, H., Knutson, H. A., Hinkley, S., Bryan, M., Crepp, J. R., Batygin, K., Crossfield, I., Hansen, B., Howard, A. W., Johnson, J. A., et al. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/827/1/8 · Cited by 158
A hot Jupiter orbiting a 2-million-year-old solar-mass T Tauri star
Donati, J. F., Moutou, C., Malo, L., Baruteau, C., Yu, L., Hébrard, E., Hussain, G., Alencar, S., Ménard, F., Bouvier, J., et al. (2016) · Nature · doi:10.1038/nature18305 · Cited by 147
Solar obliquity induced by planet nine
Bailey, E., Batygin, K., & Brown, M. E. (2016) · The Astronomical Journal · doi:10.3847/0004-6256/152/5/126 · Cited by 62
Dynamics of Planetary Systems within Star Clusters: Aspects of the Solar System’s Early Evolution
Batygin, K., Adams, F. C., Batygin, Y. K., & Petigura, E. A. (2020) · The Astronomical Journal · doi:10.3847/1538-3881/ab665d · Cited by 43
Implications of tides for life on exoplanets
Lingam, M., & Loeb, A. (2017) · arXiv · doi:10.48550/arxiv.1707.04594 · Cited by 37
Metadata
- Authors
- Winn, J. N., & Fabrycky, D. C.
- Venue
- Annual Review of Astronomy and Astrophysics
- Publisher
- Annual Reviews
- Published
- 2015-08-18
- Volume
- 53
- Issue
- 1
- Pages
- 409-447
- ISSN
- 0066-4146 (ISSN-L)
- 1545-4282
- OpenAlex
- W2130754528
- Cited by
- 891
- References
- 9
- FWCI
- 6.72
- Type
- journal article
- Language
- en
- Open access
- green
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