The KMOS3D Survey: Rotating Compact Star-forming Galaxies and the Decomposition of Integrated Line Widths

E. Wisnioski, J. T. Mendel, N. M.Förster Schreiber, R. Genzel, D. Wilman, S. Wuyts, S. Belli, A. Beifiori, R. Bender, G. Brammer, J. Chan, R. I. Davies, R. L. Davies, M. Fabricius, M. Fossati, A. Galametz, P. Lang, D. Lutz, E. J. Nelson, I. MomchevaD. Rosario, R. Saglia, L. J. Tacconi, K. Tadaki, H. Ubler, P. G. Van Dokkum

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Abstract

Using integral field spectroscopy, we investigate the kinematic properties of 35 massive centrally dense and compact star-forming galaxies (SFGs; logM[Ṁ] = 11.1, log (σ 1kpc[Ṁ kpc-2]) > 9.5 log (M∗/re 1.5 (Ṁ kpc1.5])> 10.3) at z ∼ 0.7-3.7within the KMOS3D survey. We spatially resolve 23 compact SFGs and find that the majority are dominated by rotational motions with velocities ranging from 95 to 500 km s-1. The range of rotation velocities is reflected in a similar range of integrated 1DUMMYα line widths, 75400 km s-1, consistent with the kinematic properties of mass-matched extended galaxies from the full KMOS3D sample. The fraction of compact SFGs that are classified as rotation-dominated" or "disklike" also mirrors the fractions of the full KMOS3D sample. We show that integrated lineof-sight gas velocity dispersions from KMOS3Dare best approximated by a linear combination of their rotation and turbulent velocities with a lesser but still significant contribution from galactic-scale winds. The 1DUMMYα exponential disk sizes of compact SFGs are, on average, 2.5 ± 0.2 kpc, 1-2 × the continuum sizes, in agreement with previous work. The compact SFGs have a 1.4 × higher active galactic nucleus (AGN) incidence than the full KMOS3D sample at fixed stellar mass with an average AGN fraction of 76%. Given their high and centrally concentrated stellar masses, as well as stellar-to-dynamical mass ratios close to unity, the compact SFGs are likely to have low molecular gas fractions and to quench on a short timescale unless replenished with inflowing gas. The rotation in these compact systems suggests that their direct descendants are rotating passive galaxies.

Original languageEnglish
Article number97
JournalAstrophysical Journal
Volume855
Issue number2
DOIs
Publication statusPublished - 10 Mar 2018

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decomposition
galaxies
stars
stellar mass
active galactic nuclei
kinematics
gas
visual perception
molecular gases
gases
mass ratios
spectroscopy
unity
timescale
incidence
mirrors
continuums

Keywords

  • galaxies: evolution
  • galaxies: high-redshift
  • galaxies: kinematics and dynamics
  • infrared: galaxies

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Wisnioski, E., Mendel, J. T., Schreiber, N. M. F., Genzel, R., Wilman, D., Wuyts, S., ... Van Dokkum, P. G. (2018). The KMOS3D Survey: Rotating Compact Star-forming Galaxies and the Decomposition of Integrated Line Widths. Astrophysical Journal, 855(2), [97]. https://doi.org/10.3847/1538-4357/aab097

The KMOS3D Survey : Rotating Compact Star-forming Galaxies and the Decomposition of Integrated Line Widths. / Wisnioski, E.; Mendel, J. T.; Schreiber, N. M.Förster; Genzel, R.; Wilman, D.; Wuyts, S.; Belli, S.; Beifiori, A.; Bender, R.; Brammer, G.; Chan, J.; Davies, R. I.; Davies, R. L. ; Fabricius, M.; Fossati, M.; Galametz, A.; Lang, P.; Lutz, D.; Nelson, E. J.; Momcheva, I.; Rosario, D.; Saglia, R.; Tacconi, L. J.; Tadaki, K.; Ubler, H.; Van Dokkum, P. G.

In: Astrophysical Journal, Vol. 855, No. 2, 97, 10.03.2018.

Research output: Contribution to journalArticle

Wisnioski, E, Mendel, JT, Schreiber, NMF, Genzel, R, Wilman, D, Wuyts, S, Belli, S, Beifiori, A, Bender, R, Brammer, G, Chan, J, Davies, RI, Davies, RL, Fabricius, M, Fossati, M, Galametz, A, Lang, P, Lutz, D, Nelson, EJ, Momcheva, I, Rosario, D, Saglia, R, Tacconi, LJ, Tadaki, K, Ubler, H & Van Dokkum, PG 2018, 'The KMOS3D Survey: Rotating Compact Star-forming Galaxies and the Decomposition of Integrated Line Widths', Astrophysical Journal, vol. 855, no. 2, 97. https://doi.org/10.3847/1538-4357/aab097
Wisnioski, E. ; Mendel, J. T. ; Schreiber, N. M.Förster ; Genzel, R. ; Wilman, D. ; Wuyts, S. ; Belli, S. ; Beifiori, A. ; Bender, R. ; Brammer, G. ; Chan, J. ; Davies, R. I. ; Davies, R. L. ; Fabricius, M. ; Fossati, M. ; Galametz, A. ; Lang, P. ; Lutz, D. ; Nelson, E. J. ; Momcheva, I. ; Rosario, D. ; Saglia, R. ; Tacconi, L. J. ; Tadaki, K. ; Ubler, H. ; Van Dokkum, P. G. / The KMOS3D Survey : Rotating Compact Star-forming Galaxies and the Decomposition of Integrated Line Widths. In: Astrophysical Journal. 2018 ; Vol. 855, No. 2.
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AU - Schreiber, N. M.Förster

AU - Genzel, R.

AU - Wilman, D.

AU - Wuyts, S.

AU - Belli, S.

AU - Beifiori, A.

AU - Bender, R.

AU - Brammer, G.

AU - Chan, J.

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AU - Lang, P.

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AB - Using integral field spectroscopy, we investigate the kinematic properties of 35 massive centrally dense and compact star-forming galaxies (SFGs; logM[Ṁ] = 11.1, log (σ 1kpc[Ṁ kpc-2]) > 9.5 log (M∗/re 1.5 (Ṁ kpc1.5])> 10.3) at z ∼ 0.7-3.7within the KMOS3D survey. We spatially resolve 23 compact SFGs and find that the majority are dominated by rotational motions with velocities ranging from 95 to 500 km s-1. The range of rotation velocities is reflected in a similar range of integrated 1DUMMYα line widths, 75400 km s-1, consistent with the kinematic properties of mass-matched extended galaxies from the full KMOS3D sample. The fraction of compact SFGs that are classified as rotation-dominated" or "disklike" also mirrors the fractions of the full KMOS3D sample. We show that integrated lineof-sight gas velocity dispersions from KMOS3Dare best approximated by a linear combination of their rotation and turbulent velocities with a lesser but still significant contribution from galactic-scale winds. The 1DUMMYα exponential disk sizes of compact SFGs are, on average, 2.5 ± 0.2 kpc, 1-2 × the continuum sizes, in agreement with previous work. The compact SFGs have a 1.4 × higher active galactic nucleus (AGN) incidence than the full KMOS3D sample at fixed stellar mass with an average AGN fraction of 76%. Given their high and centrally concentrated stellar masses, as well as stellar-to-dynamical mass ratios close to unity, the compact SFGs are likely to have low molecular gas fractions and to quench on a short timescale unless replenished with inflowing gas. The rotation in these compact systems suggests that their direct descendants are rotating passive galaxies.

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