A Complete ALMA Map of the Fomalhaut Debris Disk

Meredith A. Macgregor, Luca Matrà, Paul Kalas, David J. Wilner, Margaret Pan, Grant M. Kennedy, Mark C. Wyatt, Gaspard Duchene, A. Meredith Hughes, George H. Rieke, Mark Clampin, Michael P. Fitzgerald, James R. Graham, Wayne S. Holland, Olja Panić, Andrew Shannon, Kate Su

Research output: Research - peer-reviewArticle

Abstract

We present ALMA mosaic observations at 1.3 mm (223 GHz) of the Fomalhaut system with a sensitivity of 14 μJy/beam. These observations provide the first millimeter map of the continuum dust emission from the complete outer debris disk with uniform sensitivity, enabling the first conclusive detection of apocenter glow. We adopt an MCMC modeling approach that accounts for the eccentric orbital parameters of a collection of particles within the disk. The outer belt is radially confined with an inner edge of 136.3 ± 0.9 au and width of 13.5 ± 1.8 au. We determine a best-fit eccentricity of 0.12 ± 0.01. Assuming a size distribution power-law index of q = 3.46 ± 0.09, we constrain the dust absorptivity power-law index β to be 0.9 < β < 1.5. The geometry of the disk is robustly constrained with inclination 65.°6 ± 0.°3, position angle 337.°9 ± 0.°3, and argument of periastron 22.°5 ± 4.°3. Our observations do not confirm any of the azimuthal features found in previous imaging studies of the disk with Hubble Space Telescope, SCUBA, and ALMA. However, we cannot rule out structures ≤10 au in size or that only affect smaller grains. The central star is clearly detected with a flux density of 0.75 ± 0.02 mJy, significantly lower than predicted by current photospheric models. We discuss the implications of these observations for the directly imaged Fomalhaut b and the inner dust belt detected at infrared wavelengths.

LanguageEnglish (US)
Article number8
JournalAstrophysical Journal
Volume842
Issue number1
DOIs
StatePublished - Jun 10 2017

Fingerprint

debris
dust
power law
index
sensitivity
eccentricity
wavelength
geometry
modeling
parameter
mosaic
detection
particle
eccentrics
Hubble Space Telescope
inclination
absorptivity
flux density
luminescence
continuums

Keywords

  • circumstellar matter
  • stars: individual (Fomalhaut)
  • submillimeter: planetary systems

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Macgregor, M. A., Matrà, L., Kalas, P., Wilner, D. J., Pan, M., Kennedy, G. M., ... Su, K. (2017). A Complete ALMA Map of the Fomalhaut Debris Disk. Astrophysical Journal, 842(1), [8]. DOI: 10.3847/1538-4357/aa71ae

A Complete ALMA Map of the Fomalhaut Debris Disk. / Macgregor, Meredith A.; Matrà, Luca; Kalas, Paul; Wilner, David J.; Pan, Margaret; Kennedy, Grant M.; Wyatt, Mark C.; Duchene, Gaspard; Hughes, A. Meredith; Rieke, George H.; Clampin, Mark; Fitzgerald, Michael P.; Graham, James R.; Holland, Wayne S.; Panić, Olja; Shannon, Andrew; Su, Kate.

In: Astrophysical Journal, Vol. 842, No. 1, 8, 10.06.2017.

Research output: Research - peer-reviewArticle

Macgregor, MA, Matrà, L, Kalas, P, Wilner, DJ, Pan, M, Kennedy, GM, Wyatt, MC, Duchene, G, Hughes, AM, Rieke, GH, Clampin, M, Fitzgerald, MP, Graham, JR, Holland, WS, Panić, O, Shannon, A & Su, K 2017, 'A Complete ALMA Map of the Fomalhaut Debris Disk' Astrophysical Journal, vol 842, no. 1, 8. DOI: 10.3847/1538-4357/aa71ae
Macgregor MA, Matrà L, Kalas P, Wilner DJ, Pan M, Kennedy GM et al. A Complete ALMA Map of the Fomalhaut Debris Disk. Astrophysical Journal. 2017 Jun 10;842(1). 8. Available from, DOI: 10.3847/1538-4357/aa71ae
Macgregor, Meredith A. ; Matrà, Luca ; Kalas, Paul ; Wilner, David J. ; Pan, Margaret ; Kennedy, Grant M. ; Wyatt, Mark C. ; Duchene, Gaspard ; Hughes, A. Meredith ; Rieke, George H. ; Clampin, Mark ; Fitzgerald, Michael P. ; Graham, James R. ; Holland, Wayne S. ; Panić, Olja ; Shannon, Andrew ; Su, Kate. / A Complete ALMA Map of the Fomalhaut Debris Disk. In: Astrophysical Journal. 2017 ; Vol. 842, No. 1.
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