RIOJA. Complex Dusty Starbursts in a Major Merger B14-65666 at z=7.15
arxiv(2024)
摘要
We present JWST NIRCam imaging of B14-65666 ("Big Three Dragons"), a bright
Lyman-break galaxy system (M_UV=-22.5 mag) at z=7.15. The high
angular resolution of NIRCam reveals the complex morphology of two galaxy
components: galaxy E has a compact core (E-core), surrounded by diffuse,
extended, rest-frame optical emission, which is likely to be tidal tails; and
galaxy W has a clumpy and elongated morphology with a blue UV slope
(β_UV=-2.2±0.1). The flux excess, F356W-F444W, peaks at the
E-core (1.05^+0.08_-0.09 mag), tracing the presence of strong [OIII]
4960,5008 Å emission. ALMA archival data show that the bluer galaxy W is
brighter in dust continua than the redder galaxy E, while the tails are bright
in [OIII] 88 μ m. The UV/optical and sub-mm SED fitting confirms
that B14-65666 is a major merger in a starburst phase as derived from the
stellar mass ratio (3:1 to 2:1) and the star-formation rate, ≃1 dex
higher than the star-formation main sequence at the same redshift. The galaxy E
is a dusty (A_V=1.2±0.1 mag) starburst with a possible high dust
temperature (≥63-68 K). The galaxy W would have a low dust temperature
(≤27-33 K) or patchy stellar-and-dust geometry, as suggested from the
infrared excess (IRX) and β_UV diagram. The high optical-to-FIR
[OIII] line ratio of the E-core shows its lower gas-phase metallicity
(≃0.2 Z_⊙) than the galaxy W. These results agree with a
scenario where major mergers disturb morphology and induce nuclear dusty
starbursts triggered by less-enriched inflows. B14-65666 shows a picture of
complex stellar buildup processes during major mergers in the epoch of
reionization.
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