ALMA Resolves the Nuclear Disks of Arp 220

Nick Scoville, Lena Murchikova, Fabian Walter, Catherine Vlahakis, Jin Koda, Paul Vanden Bout, Joshua Barnes, Lars Hernquist, Kartik Sheth, Min Yun, David Sanders, Lee Armus, Pierre Cox, Todd Thompson, Brant E Robertson, Laura Zschaechner, Linda Tacconi, Paul Torrey, Christopher C. Hayward, Reinhard Genzel & 3 others Phil Hopkins, Paul Van Der Werf, Roberto Decarli

Research output: Contribution to journalArticle

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Abstract

We present 90 mas (37 pc) resolution ALMA imaging of Arp 220 in the CO (1-0) line and continuum at λ = 2.6 mm. The internal gas distribution and kinematics of both galactic nuclei are well resolved for the first time. In the west nucleus, the major gas and dust emission extends out to 0.″ 2 radius (74 pc); the central resolution element shows a strong peak in the dust emission but a factor of 3 dip in the CO line emission. In this nucleus, the dust is apparently optically thick (T2.6 mm ∼ 1) at λ = 2.6 mm with a dust brightness temperature of ∼147 K. The column of interstellar matter at this nucleus is NH2 ≫ 2 × 10 26 cm-2, corresponding to ∼900 gr cm-2. The east nucleus is more elongated with radial extent 0 3 or ∼111 pc. The derived kinematics of the nuclear disks provide a good fit to the line profiles, yielding the emissivity distributions, the rotation curves, and velocity dispersions. In the west nucleus, there is evidence of a central Keplerian component requiring a central mass of 8 × 108 M. The intrinsic widths of the emission lines are Δv (FWHM) = 250 (west) and 120 (east) km s-1. Given the very short dissipation timescales for turbulence (≲105 years), we suggest that the line widths may be due to semicoherent motions within the nuclear disks. The symmetry of the nuclear disk structures is impressive, implying the merger timescale is significantly longer than the rotation period of the disks.

LanguageEnglish (US)
Article number66
JournalAstrophysical Journal
Volume836
Issue number1
DOIs
StatePublished - Feb 10 2017
Externally publishedYes

Fingerprint

dust
nuclei
kinematics
timescale
interstellar matter
galactic nuclei
emissivity
gas
brightness temperature
merger
symmetry
dissipation
dip
gases
turbulence
continuums
radii
curves
profiles
distribution

Keywords

  • galaxies: active
  • galaxies: individual (Arp 220)
  • galaxies: starburst
  • Galaxy: evolution
  • ISM: clouds
  • ISM: molecules

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Scoville, N., Murchikova, L., Walter, F., Vlahakis, C., Koda, J., Bout, P. V., ... Decarli, R. (2017). ALMA Resolves the Nuclear Disks of Arp 220. Astrophysical Journal, 836(1), [66]. https://doi.org/10.3847/1538-4357/836/1/66

ALMA Resolves the Nuclear Disks of Arp 220. / Scoville, Nick; Murchikova, Lena; Walter, Fabian; Vlahakis, Catherine; Koda, Jin; Bout, Paul Vanden; Barnes, Joshua; Hernquist, Lars; Sheth, Kartik; Yun, Min; Sanders, David; Armus, Lee; Cox, Pierre; Thompson, Todd; Robertson, Brant E; Zschaechner, Laura; Tacconi, Linda; Torrey, Paul; Hayward, Christopher C.; Genzel, Reinhard; Hopkins, Phil; Werf, Paul Van Der; Decarli, Roberto.

In: Astrophysical Journal, Vol. 836, No. 1, 66, 10.02.2017.

Research output: Contribution to journalArticle

Scoville, N, Murchikova, L, Walter, F, Vlahakis, C, Koda, J, Bout, PV, Barnes, J, Hernquist, L, Sheth, K, Yun, M, Sanders, D, Armus, L, Cox, P, Thompson, T, Robertson, BE, Zschaechner, L, Tacconi, L, Torrey, P, Hayward, CC, Genzel, R, Hopkins, P, Werf, PVD & Decarli, R 2017, 'ALMA Resolves the Nuclear Disks of Arp 220' Astrophysical Journal, vol. 836, no. 1, 66. https://doi.org/10.3847/1538-4357/836/1/66
Scoville N, Murchikova L, Walter F, Vlahakis C, Koda J, Bout PV et al. ALMA Resolves the Nuclear Disks of Arp 220. Astrophysical Journal. 2017 Feb 10;836(1). 66. https://doi.org/10.3847/1538-4357/836/1/66
Scoville, Nick ; Murchikova, Lena ; Walter, Fabian ; Vlahakis, Catherine ; Koda, Jin ; Bout, Paul Vanden ; Barnes, Joshua ; Hernquist, Lars ; Sheth, Kartik ; Yun, Min ; Sanders, David ; Armus, Lee ; Cox, Pierre ; Thompson, Todd ; Robertson, Brant E ; Zschaechner, Laura ; Tacconi, Linda ; Torrey, Paul ; Hayward, Christopher C. ; Genzel, Reinhard ; Hopkins, Phil ; Werf, Paul Van Der ; Decarli, Roberto. / ALMA Resolves the Nuclear Disks of Arp 220. In: Astrophysical Journal. 2017 ; Vol. 836, No. 1.
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AU - Bout, Paul Vanden

AU - Barnes, Joshua

AU - Hernquist, Lars

AU - Sheth, Kartik

AU - Yun, Min

AU - Sanders, David

AU - Armus, Lee

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AB - We present 90 mas (37 pc) resolution ALMA imaging of Arp 220 in the CO (1-0) line and continuum at λ = 2.6 mm. The internal gas distribution and kinematics of both galactic nuclei are well resolved for the first time. In the west nucleus, the major gas and dust emission extends out to 0.″ 2 radius (74 pc); the central resolution element shows a strong peak in the dust emission but a factor of 3 dip in the CO line emission. In this nucleus, the dust is apparently optically thick (T2.6 mm ∼ 1) at λ = 2.6 mm with a dust brightness temperature of ∼147 K. The column of interstellar matter at this nucleus is NH2 ≫ 2 × 10 26 cm-2, corresponding to ∼900 gr cm-2. The east nucleus is more elongated with radial extent 0 3 or ∼111 pc. The derived kinematics of the nuclear disks provide a good fit to the line profiles, yielding the emissivity distributions, the rotation curves, and velocity dispersions. In the west nucleus, there is evidence of a central Keplerian component requiring a central mass of 8 × 108 M⊙. The intrinsic widths of the emission lines are Δv (FWHM) = 250 (west) and 120 (east) km s-1. Given the very short dissipation timescales for turbulence (≲105 years), we suggest that the line widths may be due to semicoherent motions within the nuclear disks. The symmetry of the nuclear disk structures is impressive, implying the merger timescale is significantly longer than the rotation period of the disks.

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KW - galaxies: starburst

KW - Galaxy: evolution

KW - ISM: clouds

KW - ISM: molecules

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