Predictions for a planet just inside Fomalhaut's eccentric ring
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17 citations
Cites background from "Predictions for a planet just insid..."
...Resolved images of disks show that features such as sharp radial profiles, warps, clumps, and spirals can be caused by unseen planets (Quillen 2006a; Nesvold & Kuchner 2015)....
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...Models of observable disk features have led to the discoveries of directly imaged planets around their host stars such as β-Pictoris b (Lagrange et al. 2010) and Fomalhaut b (Quillen 2006b)....
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16 citations
Additional excerpts
...According to Quillen (2006), a body is captured into the 2:1 resonance when its ini- tial eccentricity is below a certain limit given byelim ∼ 1.5µ1/3....
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16 citations
Cites background from "Predictions for a planet just insid..."
...The separation of the planet from the disk is sensitive to the planet mass, as the planet clears a chaotic zone around itself due to resonance overlap (e.g. Quillen 2006; Chiang et al. 2009)....
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14 citations
14 citations
Cites background from "Predictions for a planet just insid..."
...Such an interaction can manifest as a warp (e.g., Beta Pic; Burrows et al. 1995; Mouillet et al. 1997), a stellocentric offset (e.g., HR 4796A; Wyatt et al. 1999; Telesco et al. 2000), or a sharp radial profile at the inner edge of a dust ring (e.g., Fomalhaut; Kalas et al. 2005; Quillen 2006)....
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References
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"Predictions for a planet just insid..." refers background in this paper
...2 T H E P E R I C E N T R E G L OW M O D E L A N D A N E C C E N T R I C E D G E I N F O M A L H AU T ’ S D I S C We follow the theory for secular perturbations induced by a planet (e.g. Murray & Dermott 1999; Wyatt et al. 1999)....
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...Secular perturbations in the plane can be described in terms of the complex eccentricity variable, z = e exp(i ), where e is the object’s eccentricity and is its longitude of periastron (e.g. Murray & Dermott 1999; Wyatt et al. 1999)....
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...The functions, b js (α), are Laplace coefficients (see Murray & Dermott 1999 for definitions and numerical expressions)....
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...The time variation of z is ż = zforced + zproper(t) (1) where zforced = b23/2(α) b13/2(α) ep exp(i p) (2) (Murray & Dermott 1999; Wyatt et al. 1999)....
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1,601 citations
"Predictions for a planet just insid..." refers background or methods in this paper
...(4) We have recovered the scaling with planet mass predicted by previous works (Goldreich & Tremaine 1980; Franklin et al. 1980; Lissauer & Espresate 1998) but have also included a dependence on distance from the planet....
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...Franklin et al. (1980), Goldreich & Tremaine (1980) and Lissauer & Espresate (1998) showed that spiral density waves were efficiently driven at a Lindblad resonance by a satellite when the collision time-scale was above a critical one, t crit, where t crit ∝ μ−2/3, and μ ≡ m p/M ∗ is the ratio of…...
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488 citations
"Predictions for a planet just insid..." refers background in this paper
...The width of this zone has been measured numerically and predicted theoretically for a planet in a circular orbit by predicting the semi-major axis at which the first-order mean motion resonances overlap (Wisdom 1980; Duncan, Quinn & Tremaine 1989; Murray & Holman 1997; Mudryk & Wu 2006)....
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459 citations
"Predictions for a planet just insid..." refers background in this paper
...1 I N T RO D U C T I O N The nearby star Fomalhaut hosts a ring of circumstellar material (Aumann 1985; Gillett 1985) residing between 120 and 160 au from the star (Holland et al. 1998; Dent et al. 2000; Holland et al. 2003)....
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