The DOI matches its Crossref record; 148 of the 148 references it cites were found in a registry or an index.
THE ROLE OF MULTIPLICITY IN DISK EVOLUTION AND PLANET FORMATION
Open accessAbstract
The past decade has seen a revolution in our understanding of protoplanetary disk evolution and planet formation in single-star systems. However, the majority of solar-type stars form in binary systems, so the impact of binary companions on protoplanetary disks is an important element in our understanding of planet formation. We have compiled a combined multiplicity/disk census of Taurus–Auriga, plus a restricted sample of close binaries in other regions, in order to explore the role of multiplicity in disk evolution. Our results imply that the tidal influence of a close (≲40 AU) binary companion significantly hastens the process of protoplanetary disk dispersal, as ∼2/3 of all close binaries promptly disperse their disks within ≲1 Myr after formation. However, prompt disk dispersal only occurs for a small fraction of wide binaries and single stars, with ∼80%–90% retaining their disks for at least ∼2–3 Myr (but rarely for more than ∼5 Myr). Our new constraints on the disk clearing timescale have significant implications for giant planet formation; most single stars have 3–5 Myr within which to form giant planets, whereas most close binary systems would have to form giant planets within ≲1 Myr. If core accretion is the primary mode for giant planet formation, then gas giants in close binaries should be rare. Conversely, since almost all single stars have a similar period of time within which to form gas giants, their relative rarity in radial velocity (RV) surveys indicates either that the giant planet formation timescale is very well matched to the disk dispersal timescale or that features beyond the disk lifetime set the likelihood of giant planet formation.
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Cites
On the Gravitational Stability of a Disk of Stars
Toomre, A. (1964) · The Astrophysical Journal · doi:10.1086/147861 · Cited by 3,349 · cited 1×
“The two canonical modes proposed for gas giant formation are the assembly of a rockice core that can accrete and hold gas (“core accretion”; Pollack et al. 1996) and the direct fragmentation and collapse of material in a Toomre-unstable disk (“disk instability”; Toomre 1964; Boss 2001).”
BackgroundFormation of the Giant Planets by Concurrent Accretion of Solids and Gas
Pollack, J. B., Hubickyj, O., Bodenheimer, P., Lissauer, J. J., Podolak, M., & Greenzweig, Y. (1996) · Icarus · doi:10.1006/icar.1996.0190 · Cited by 3,127
Star Formation in Molecular Clouds: Observation and Theory
Shu, F. H., Adams, F. C., & Lizano, S. (1987) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.aa.25.090187.000323 · Cited by 2,388
Aerodynamics of solid bodies in the solar nebula
Weidenschilling, S. J. (1977) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/180.2.57 · Cited by 1,984
A SURVEY OF STELLAR FAMILIES: MULTIPLICITY OF SOLAR-TYPE STARS
Raghavan, D., McAlister, H. A., Henry, T. J., Latham, D. W., Marcy, G. W., Mason, B. D., Gies, D. R., White, R. J., & ten Brummelaar, T. A. (2010) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/190/1/1 · Cited by 1,853
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
Accretion and the Evolution of T Tauri Disks
Hartmann, L., Calvet, N., Gullbring, E., & D'Alessio, P. (1998) · The Astrophysical Journal · doi:10.1086/305277 · Cited by 1,569
Dynamics of binary-disk interaction. 1: Resonances and disk gap sizes
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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
Disk Accretion and Mass Loss from Young Stars
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Cited by
AN OPTICAL SPECTROSCOPIC STUDY OF T TAURI STARS. I. PHOTOSPHERIC PROPERTIES
Herczeg, G. J., & Hillenbrand, L. A. (2014) · The Astrophysical Journal · doi:10.1088/0004-637x/786/2/97 · Cited by 447
Self-citationNgo, 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
THE EVOLUTION OF STELLAR ROTATION AND THE HYDROGEN ATMOSPHERES OF HABITABLE-ZONE TERRESTRIAL PLANETS
Johnstone, C. P., Güdel, M., Stökl, A., Lammer, H., Tu, L., Kislyakova, K. G., Lüftinger, T., Odert, P., Erkaev, N. V., & Dorfi, E. A. (2015) · The Astrophysical Journal · doi:10.1088/2041-8205/815/1/l12 · Cited by 151
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
Ngo, H., Knutson, H. A., Bryan, M. L., Blunt, S., Nielsen, E. L., Batygin, K., Bowler, B. P., Crepp, J. R., Hinkley, S., Howard, A. W., et al. (2017) · The Astronomical Journal · doi:10.3847/1538-3881/aa6cac · Cited by 28
Metadata
- Authors
- Kraus, A. L., Ireland, M. J., Hillenbrand, L. A., & Martinache, F.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2011-12-28
- Volume
- 745
- Issue
- 1
- Pages
- 19
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W1989828771
- Cited by
- 280
- References
- 148
- FWCI
- 10.37
- Type
- journal article
- Language
- en
- Open access
- bronze
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- Kraus, A. L., Ireland, M. J., Hillenbrand, L. A., & Martinache, F. (2012). THE ROLE OF MULTIPLICITY IN DISK EVOLUTION AND PLANET FORMATION. The Astrophysical Journal. https://doi.org/10.1088/0004-637x/745/1/19
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