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ALMA Reveals Metals yet No Dust within Multiple Components in CR7

Matthee, J. (författare)
Sobral, D. (författare)
Boone, F. (författare)
visa fler...
Rottgering, H. (författare)
Schaerer, D. (författare)
Girard, M. (författare)
Pallottini, A. (författare)
Vallini, Livia (författare)
Stockholms universitet,Nordiska institutet för teoretisk fysik (Nordita),Stockholms universitet, Sverige; Nordita SU
Ferrara, A. (författare)
Darvish, B. (författare)
Mobasher, B. (författare)
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 (creator_code:org_t)
2017-12-21
2017
Engelska.
Ingår i: Astrophysical Journal. - : Institute of Physics Publishing (IOPP). - 0004-637X .- 1538-4357. ; 851:2
  • Tidskriftsartikel (refereegranskat)
Abstract Ämnesord
Stäng  
  • We present spectroscopic follow-up observations of CR7 with ALMA, targeted at constraining the infrared (IR) continuum and [C II](158 mu m) line-emission at high spatial resolution matched to the HST/WFC3 imaging. CR7 is a luminous Ly alpha emitting galaxy at z = 6.6 that consists of three separated UV-continuum components. Our observations reveal several well-separated components of [C II] emission. The two most luminous components in [C II] coincide with the brightest UV components (A and B), blueshifted by approximate to 150 km s(-1) with respect to the peak of Lya emission. Other [C II] components are observed close to UV clumps B and C and are blueshifted by approximate to 300 and approximate to 80 km s(-1) with respect to the systemic redshift. We do not detect FIR continuum emission due to dust with a 3 sigma limiting luminosity L-IR(T-d = 35 K) < 3.1 x 10(10) L-circle dot. This allows us to mitigate uncertainties in the dust-corrected SFR and derive SFRs for the three UV clumps A, B, and C of 28, 5, and 7 M-circle dot yr(-1). All clumps have [C II] luminosities consistent within the scatter observed in the local relation between SFR and L[C II], implying that strong Ly alpha emission does not necessarily anti-correlate with [C II] luminosity. Combining our measurements with the literature, we show that galaxies with blue UV slopes have weaker [C II] emission at fixed SFR, potentially due to their lower metallicities and/or higher photoionization. Comparison with hydrodynamical simulations suggests that CR7's clumps have metallicities of 0.1 < Z/Z(circle dot) < 0.2. The observed ISM structure of CR7 indicates that we are likely witnessing the build up of a central galaxy in the early universe through complex accretion of satellites.

Ämnesord

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
NATURVETENSKAP  -- Fysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences (hsv//eng)

Nyckelord

dark ages
reionization
first stars
galaxies: formation
galaxies: high-redshift
galaxies: ISM
galaxies: kinematics and dynamics

Publikations- och innehållstyp

ref (ämneskategori)
art (ämneskategori)

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