2003ApJ...588.1110K

Query : 2003ApJ...588.1110K

2003ApJ...588.1110K - Astrophys. J., 588, 1110-1120 (2003/May-2)

The geometry of resonant signatures in debris disks with planets.

KUCHNER M.J. and HOLMAN M.J.

Abstract (from CDS):

Using simple geometrical arguments, we paint an overview of the variety of resonant structures a single planet with moderate eccentricity (e≲0.6) can create in a dynamically cold, optically thin dust disk. This overview may serve as a key for interpreting images of perturbed debris disks and inferring the dynamical properties of the planets responsible for the perturbations. We compare the resonant geometries found in the solar system dust cloud with observations of dust clouds around Vega, ε Eridani, and Fomalhaut.

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Journal keyword(s): Celestial Mechanics - Stars: Circumstellar Matter - Interplanetary Medium - Stars: Planetary Systems - Stars: Individual: Constellation Name: α Lyrae - Stars: Individual: Constellation Name: ε Eridani - Stars: Individual: Name: Fomalhaut

Simbad objects: 4

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Number of rows : 4
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 * eps Eri BY* 03 32 55.8444911587 -09 27 29.739493865 5.19 4.61 3.73 3.00 2.54 K2V 2073 1
2 * bet Pic PM* 05 47 17.0876901 -51 03 59.441135 4.13 4.03 3.86 3.74 3.58 A6V 2087 1
3 * alf Lyr dS* 18 36 56.33635 +38 47 01.2802 0.03 0.03 0.03 0.07 0.10 A0V 2787 1
4 * alf PsA PM* 22 57 39.04625 -29 37 20.0533 1.31 1.25 1.16 1.11 1.09 A4V 1303 3

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