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ALMA Reveals Metals...
ALMA Reveals Metals yet No Dust within Multiple Components in CR7
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Matthee, J. (författare)
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Sobral, D. (författare)
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Boone, F. (författare)
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Rottgering, H. (författare)
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Schaerer, D. (författare)
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Girard, M. (författare)
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Pallottini, A. (författare)
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- Vallini, Livia (författare)
- Stockholms universitet,Nordiska institutet för teoretisk fysik (Nordita),Stockholms universitet, Sverige; Nordita SU
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Ferrara, A. (författare)
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Darvish, B. (författare)
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Mobasher, B. (författare)
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(creator_code:org_t)
- 2017-12-21
- 2017
- Engelska.
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Ingår i: Astrophysical Journal. - : Institute of Physics Publishing (IOPP). - 0004-637X .- 1538-4357. ; 851:2
- Relaterad länk:
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https://doi.org/10.3...
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https://authors.libr...
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https://urn.kb.se/re...
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https://doi.org/10.3...
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https://urn.kb.se/re...
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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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Till lärosätets databas
- Av författaren/redakt...
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Matthee, J.
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Sobral, D.
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Boone, F.
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Rottgering, H.
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Schaerer, D.
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Girard, M.
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visa fler...
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Pallottini, A.
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Vallini, Livia
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Ferrara, A.
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Darvish, B.
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Mobasher, B.
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visa färre...
- Om ämnet
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- NATURVETENSKAP
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NATURVETENSKAP
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NATURVETENSKAP
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Astrophysical Jo ...
- Av lärosätet
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Kungliga Tekniska Högskolan
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Stockholms universitet