The DOI matches its Crossref record; 5 of the 5 references it cites were found in a registry or an index.
LUNAR ACCRETION FROM A ROCHE-INTERIOR FLUID DISK
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In the citing paper
“Additionally, larger disks might produce other moonlets (Rufu et al. 2017;Citron et al. 2018b), and satellites may accrete significant additional material from the debris disk (Salmon & Canup 2012;Lock et al. 2018).”
From Immediate Origin of the Moon as a Post-impact Satellite (2022) · cites this paper as Salmon & Canup 2012
In the citing paper
“The lunar volatile signature may be difficult to reproduce without a prolonged disk phase (Dauphas et al. 2022), but loss from a magma ocean might be sufficient (Day et al. 2020), and significant disk material could also be later accreted onto the satellite's sampled exterior (Salmon & Canup 2012;Citron et al. 2018b).”
From Immediate Origin of the Moon as a Post-impact Satellite (2022) · cites this paper as Salmon & Canup 2012
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Citations
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×
“Indeed, its Toomre parameter is (Toomre 1964) Q = csΩ πGσ ≈ 52 ( rd R⊕ )−3/2( T 2000 K )1/2( σ 107 g cm−2 )−1 , (3) where T is the disk’s temperature and cs = √ γRT/µ, γ = 1.4 is the adiabatic index, R is the universal gas constant and µ = 30 g mol−1 is the molecular weight.”
InfluentialOrigin of the Moon in a giant impact near the end of the Earth's formation
Canup, R. M., & Asphaug, E. (2001) · Nature · doi:10.1038/35089010 · Cited by 1,094 · cited 1×
“…that the impactor is destroyed (either during the impact, or via post-impact tidal disruption), and that a circumterrestrial disk is formed that contains up to ∼ 2MK of iron-depleted material (Benz et al. 1986, 1987, 1989; Cameron & Benz 1991; Cameron 1997; Canup & Asphaug 2001; Canup 2004, 2008).”
BackgroundSelf-citationSimulations of a late lunar-forming impact
Canup, R. M. (2004) · Icarus · doi:10.1016/j.icarus.2003.09.028 · Cited by 669
Self-citationEquilibration in the aftermath of the lunar-forming giant impact
Pahlevan, K., & Stevenson, D. J. (2007) · Earth and Planetary Science Letters · doi:10.1016/j.epsl.2007.07.055 · Cited by 381
Lunar-forming collisions with pre-impact rotation
CANUP, R. (2008) · Icarus · doi:10.1016/j.icarus.2008.03.011 · Cited by 157
Self-citation
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Cited by
Forming a Moon with an Earth-like composition via a giant impact
Canup, R. M. (2012) · Science · doi:10.1126/science.1226073 · Cited by 656
Immediate Origin of the Moon as a Post-impact Satellite
Kegerreis, J. A., Ruiz-Bonilla, S., Eke, V. R., Massey, R. J., Sandnes, T. D., & Teodoro, L. F. A. (2022) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/ac8d96 · Cited by 50
Metadata
- Authors
- Salmon, J., & Canup, R. M.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2012-11-07
- Volume
- 760
- Issue
- 1
- Pages
- 83
- ISSN
- 0004-637X
- 1538-4357
- Cited by
- 110
- References
- 5
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- CoChat. (2026). Citation check: LUNAR ACCRETION FROM A ROCHE-INTERIOR FLUID DISK. https://app.cochat.ai/papers/10.1088/0004-637x/760/1/83
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- Salmon, J., & Canup, R. M. (2012). LUNAR ACCRETION FROM A ROCHE-INTERIOR FLUID DISK. The Astrophysical Journal. https://doi.org/10.1088/0004-637x/760/1/83
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Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
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.
