ALMA Resolves the Nuclear Disks of Arp 220

作者：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; Zschaechner Laura; Tacconi Linda; Torrey Paul; Hayward Christopher C; Genzel Reinhard; Hopkins Phil; van der Werf Paul; Decarli Roberto

来源：Astrophysical Journal, 2017, 836(1): 66.

DOI：10.3847/1538-4357/836/1/66

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

We present 90 mas (37 pc) resolution ALMA imaging of Arp 220 in the CO (1-0) line and continuum at gimel = 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 (tau(2.6) mm similar to 1) at lambda = 2.6 mm with a dust brightness temperature of similar to 147 K. The column of interstellar matter. at this nucleus is NH2. 2 x 10(26) cm(-2), corresponding to similar to 900 gr cm(-2). The east nucleus is more elongated with radial extent 0 3 or similar to 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 x 10(8) M-circle dot. The intrinsic widths of the emission lines are Delta v(FWHM)= 250 (west) and 120 (east) km s(-1). Given the very short dissipation timescales for turbulence (less than or similar to 10(5) 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.

• 出版日期2017-2-10
• 单位MIT