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Detailed study of stars and gas in a z = 8.3 massive merger with extreme dust conditions
ID
Harshan, Anishya
(
Author
),
ID
Tripodi, Roberta
(
Author
),
ID
Martis, Nicholas S.
(
Author
),
ID
Rihtaršič, Gregor
(
Author
),
ID
Bradač, Maruša
(
Author
),
ID
Markov, Vladan
(
Author
), et al.
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https://iopscience.iop.org/article/10.3847/2041-8213/ad9741
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Abstract
We present galaxy MACS0416-Y1 at z$_{spec}$ = 8.312 as observed by the CAnadian NIRISS Unbiased Cluster Survey. MACS0416-Y1 has been shown to have extreme dust properties; thus, we study the physical properties and star formation histories of its resolved components. Overall, we find that MACS0416-Y1 is undergoing a star formation burst in three resolved clumps. The central clump is less massive compared to the other clumps and possibly formed in the merging process of the two larger clumps. Although the star formation history indicates an ongoing star formation burst, this gas-rich galaxy shows comparable star formation efficiency to cosmic noon galaxies. Using NIRSpec prism spectroscopy, we measure metallicity, 12 + log (O/H) = 7.76 ± 0.03, ionization parameter, log U = –2.48 ± 0.03, and electron temperature T$_e$ = 18000 ± 4000 K. The emission line ratios of the galaxy indicate an evolved interstellar medium similar to z ∼ 2 star-forming galaxies. Further, we find possible presence of ionization from an active galactic nucleus (AGN) using emission line diagnostics; however, we do not detect a broad-line component in the Hβ emission line. As this gas-rich galaxy is undergoing a major merger, we hypothesize that the high dust temperature in MACS0416-Y1 is caused by the star formation burst or a possible narrow-line AGN.
Language:
English
Keywords:
high-redshift galaxies
,
gravitational lensing
,
reionization
,
active galaxies
,
strong gravitational lensing
Work type:
Article
Typology:
1.01 - Original Scientific Article
Organization:
FMF - Faculty of Mathematics and Physics
Publication status:
Published
Publication version:
Version of Record
Year:
2024
Number of pages:
9 str.
Numbering:
Vol. 977, no. 2, art. L36
PID:
20.500.12556/RUL-166375
UDC:
524.8
ISSN on article:
2041-8213
DOI:
10.3847/2041-8213/ad9741
COBISS.SI-ID:
221495555
Publication date in RUL:
09.01.2025
Views:
559
Downloads:
166
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Record is a part of a journal
Title:
The Astrophysical journal. Letters
Shortened title:
Astrophys. J. Lett.
Publisher:
American Astronomical Society
ISSN:
2041-8213
COBISS.SI-ID:
367233
Licences
License:
CC BY 4.0, Creative Commons Attribution 4.0 International
Link:
http://creativecommons.org/licenses/by/4.0/
Description:
This is the standard Creative Commons license that gives others maximum freedom to do what they want with the work as long as they credit the author.
Projects
Funder:
EC - European Commission
Funding programme:
HE
Project number:
101053208
Name:
Exploring Cosmic Dawn with James Webb Space Telescope
Acronym:
FIRSTLIGHT
Funder:
ARRS - Slovenian Research Agency
Project number:
N1-0238
Name:
Raziskave kozmične zore z James Webb vesoljskim teleskopom
Funder:
ARRS - Slovenian Research Agency
Project number:
P1-0188
Name:
Astrofizika in fizika atmosfere
Funder:
NASA, STScI
Funding programme:
HST-GO-16667
Project number:
NAS5-26555
Funder:
Canadian Space Agency
Project number:
18JWST-GTO1
Funder:
Natural Sciences and Engineering Research Council of Canada
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