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VLA and ALMA Imaging of Intense, Galaxy-Wide Star Formation in z ~ 2 Galaxies

Research output: Contribution to journalArticle

  • W. Rujopakarn
  • G. H. Rieke
  • A. Cibinel
  • K. Nyland
  • P. Jagannathan
  • J. D. Silverman
  • A. D. Biggs
  • S. Bhatnagar
  • D. R. Ballantyne
  • M. Dickinson
  • D. Elbaz
  • J. E. Geach
  • A. Kirkpatrick
  • D. Narayanan
  • F. N. Owen
  • M. Pannella
  • C. Papovich
  • U. Rau
  • B. E. Robertson
  • A. M. Swinbank
  • P. van der Werf
  • E. van Kampen
  • B. J. Weiner
  • R. A. Windhorst

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Open

Documents

http://adsabs.harvard.edu/abs/2016arXiv160707710R
Original languageEnglish
JournalAstrophysical Journal
Volume833
Issue number1
StatePublished - 1 Dec 2016

Abstract

We present $\simeq$0$.\!\!^{\prime\prime}4$-resolution extinction-independent distributions of star formation and dust in 11 star-forming galaxies (SFGs) at $z = 1.3-3.0$. These galaxies are selected from sensitive, blank-field surveys of the $2' \times 2'$ Hubble Ultra-Deep Field at $\lambda = 5$ cm and 1.3 mm using the Karl G. Jansky Very Large Array (VLA) and Atacama Large Millimeter/submillimeter Array (ALMA). They have star-formation rates (SFRs), stellar masses, and dust properties representative of massive main-sequence SFGs at $z \sim 2$. Morphological classification performed on spatially-resolved stellar mass maps indicates a mixture of disk and morphologically disturbed systems; half of the sample harbor X-ray active galactic nuclei (AGN), thereby representing a diversity of $z \sim 2$ SFGs undergoing vigorous mass assembly. We find that their intense star formation most frequently occurs at the location of stellar-mass concentration and extends over an area comparable to their stellar-mass distribution, with a median diameter of $4.2 \pm 1.8$ kpc. This provides direct evidence for galaxy-wide star formation in distant, blank-field-selected main-sequence SFGs. The typical galactic-average SFR surface density is 2.5 M$_{\odot}$yr$^{-1}$kpc$^{-2}$, sufficiently high to drive outflows. In X-ray-selected AGN where radio emission is enhanced over the level associated with star formation, the radio excess pinpoints the AGN, which are found to be co-spatial with star formation. The median extinction-independent size of main-sequence SFGs is two times larger than those of bright submillimeter galaxies whose SFRs are $3-8$ times larger, providing a constraint on the characteristic SFR ($\sim300$ M$_{\odot}$yr$^{-1}$) above which a significant population of more compact star-forming galaxies appears to emerge.

Research areas

  • Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics

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