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Molecular gas in AzTEC/C159: a star-forming disk galaxy 1.3 Gyr after the Big Bang

Jiménez-Andrade, E.F.; Magnelli, B.; Karim, A.; Jones, G.C.; Carilli, C.L.; Romano-Díaz, E.; Gómez-Guijarro, C.; Toft, S.; Bertoldi, F.; Riechers, D.A.; Schinnerer, E.; Sargent, M.; Michałowski, M.J.; Fraternali, F.; Staguhn, J.G.; Smolčić, V.; Aravena, M.; Harrington, K.C.; Sheth, K.; Capak, P.L.; Koekemoer, A.M.; van Kampen, E.; Swinbank, M.; Zirm, A.; Magdis, G.E.; Navarrete, F.

Molecular gas in AzTEC/C159: a star-forming disk galaxy 1.3 Gyr after the Big Bang Thumbnail


Authors

E.F. Jiménez-Andrade

B. Magnelli

A. Karim

G.C. Jones

C.L. Carilli

E. Romano-Díaz

C. Gómez-Guijarro

S. Toft

F. Bertoldi

D.A. Riechers

E. Schinnerer

M. Sargent

M.J. Michałowski

F. Fraternali

J.G. Staguhn

V. Smolčić

M. Aravena

K.C. Harrington

K. Sheth

P.L. Capak

A.M. Koekemoer

E. van Kampen

A. Zirm

G.E. Magdis

F. Navarrete



Abstract

We studied the molecular gas properties of AzTEC/C159, a star-forming disk galaxy at z = 4.567, in order to better constrain the nature of the high-redshift end of the submillimeter-selected galaxy (SMG) population. We secured 12CO molecular line detections for the J = 2 →1 and J = 5 →4 transitions using the Karl G. Jansky Very Large Array (VLA) and the NOrthern Extended Millimeter Array (NOEMA) interferometer. The broad (FWHM ~ 750 km s−1) and tentative double-peaked profiles of the two 12CO lines are consistent with an extended molecular gas reservoir, which is distributed in a rotating disk, as previously revealed from [CII] 158 μm line observations. Based on the 12CO(2 →1) emission line, we derived L′CO=(3.4±0.6)×1010 K km s−1 pc2, which yields a molecular gas mass of MH2(αCO/4.3)=(1.5±0.3)×1011 M⊙ and unveils a gas-rich system with μgas(αCO/4.3)≡MH2/M⋆=3.3±0.7. The extreme star formation efficiency of AzTEC/C159, parametrized by the ratio LIR/L′CO=(216±80) L⊙ (K km s−1 pc2)−1, is comparable to merger-driven starbursts such as local ultra-luminous infrared galaxies and SMGs. Likewise, the 12CO(5 →4)/CO(2 →1) line brightness temperature ratio of r52 = 0.55 ± 0.15 is consistent with high-excitation conditions as observed in SMGs. Based on mass budget considerations, we constrained the value for the L′CO – H2 mass conversion factor in AzTEC/C159, that is, αCO=3.9−1.3+2.7 M⊙ K−1 km−1 s pc−2, which is consistent with a self-gravitating molecular gas distribution as observed in local star-forming disk galaxies. Cold gas streams from cosmological filaments might be fueling a gravitationally unstable gas-rich disk in AzTEC/C159, which breaks into giant clumps and forms stars as efficiently as in merger-driven systems and generates high gas excitation. These results support the evolutionary connection between AzTEC/C159-like systems and massive quiescent disk galaxies at z ~ 2.

Journal Article Type Article
Acceptance Date Feb 9, 2018
Online Publication Date Jul 5, 2018
Publication Date Jul 5, 2018
Deposit Date Jul 20, 2018
Publicly Available Date Jul 20, 2018
Journal Astronomy and astrophysics.
Print ISSN 0004-6361
Electronic ISSN 1432-0746
Publisher EDP Sciences
Peer Reviewed Peer Reviewed
Volume 615
Article Number A25
DOI https://doi.org/10.1051/0004-6361/201732186
Public URL https://durham-repository.worktribe.com/output/1325666

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Copyright Statement
Reproduced with permission from Astronomy & Astrophysics, © ESO 2018






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