Details

Autor(en) / Beteiligte

• Liu, Daizhong
• Schreiber, N. M. Förster
• Genzel, R.
• Lutz, D.
• Price, S. H.
• Lee, L. L.
• Baker, Andrew J.
• Burkert, A.
• Coogan, R. T.
• Davies, R. I.
• Davies, R. L.
• Herrera-Camus, R.
• Kodama, Tadayuki
• Lee, Minju M.
• Nestor, A.
• Pulsoni, C.
• Renzini, A.
• Sharon, Chelsea E.
• Shimizu, T. T.
• Tacconi, L. J.
• Tadaki, Ken-ichi
• Übler, H.

Titel

An ∼600 pc View of the Strongly Lensed, Massive Main-sequence Galaxy J0901: A Baryon-dominated, Thick Turbulent Rotating Disk with a Clumpy Cold Gas Ring at z = 2.259

Ist Teil von

• The Astrophysical journal, 2023-01, Vol.942 (2), p.98

Ort / Verlag

Philadelphia: The American Astronomical Society

Erscheinungsjahr

2023

Quelle

EZB Electronic Journals Library

Beschreibungen/Notizen

• Abstract We present a high-resolution kinematic study of the massive main-sequence star-forming galaxy (SFG) SDSS J090122.37+181432.3 (J0901) at z = 2.259, using ∼0.″36 Atacama Large Millimeter/submillimeter Array CO(3–2) and ∼0.″1–0.″5 SINFONI/VLT H α observations. J0901 is a rare, strongly lensed but otherwise normal massive ( log ( M ⋆ / M ⊙ ) ∼ 11 ) main-sequence SFG, offering a unique opportunity to study a typical massive SFG under the microscope of lensing. Through forward dynamical modeling incorporating lensing deflection, we fit the CO and H α kinematics in the image plane out to about one disk effective radius ( R e ∼ 4 kpc) at an ∼600 pc delensed physical resolution along the kinematic major axis. Our results show high intrinsic dispersions of the cold molecular and warm ionized gas ( σ 0,mol. ∼ 40 km s −1 and σ 0,ion. ∼ 66 km s −1 ) that remain constant out to R e ; a moderately low dark matter fraction ( f DM ∼ 0.3–0.4) within R e ; and a centrally peaked Toomre Q parameter—agreeing well with the previously established σ 0 versus z , f DM versus Σ baryon , and Q 's radial trends using large-sample non-lensed main-sequence SFGs. Our data further reveal a high stellar mass concentration within ∼1–2 kpc with little molecular gas, and a clumpy molecular gas ring-like structure at R ∼ 2–4 kpc, in line with the inside-out quenching scenario. Our further analysis indicates that J0901 had assembled half of its stellar mass only ∼400 Myr before its observed cosmic time, and the cold gas ring and dense central stellar component are consistent with signposts of a recent wet compaction event of a highly turbulent disk found in recent simulations.