The ALPINE-ALMA [C ii ] survey: characterization of spatial offsets in main-sequence galaxies at z ∼ 4–6
Article Swipe
Meghana Killi
,
M. Ginolfi
,
Gergö Popping
,
D. Watson
,
G. Zamorani
,
B. C. Lemaux
,
Seiji Fujimoto
,
Andreas L. Faisst
,
M. Béthermin
,
Michael Romano
,
Yoshinobu Fudamoto
,
S. Bardelli
,
M. Boquien
,
Stefano Carniani
,
M. Dessauges‐Zavadsky
,
C. Gruppioni
,
Nimish P. Hathi
,
E. Ibar
,
Gareth C. Jones
,
Anton M. Koekemoer
,
Ivanna Langan
,
Hugo Méndez-Hernández
,
Yuma Sugahara
,
L. Vallini
,
D. Vergani
·
YOU?
·
· 2024
· Open Access
·
· DOI: https://doi.org/10.1093/mnras/stae1371
YOU?
·
· 2024
· Open Access
·
· DOI: https://doi.org/10.1093/mnras/stae1371
The morphology of galaxies is shaped by stellar activity, feedback, gas and dust properties, and interactions with surroundings, and can therefore provide insight into these processes. In this paper, we study the spatial offsets between stellar and interstellar medium emission in a sample of 54 main-sequence star-forming galaxies at z ∼ 4–6 observed with the Atacama Large Millimeter/submillimeter Array (ALMA), and drawn from the ALMA Large Program to INvestigate C+ at Early times (ALPINE). We find no significant spatial offset for the majority (∼70 per cent) of galaxies in the sample among any combination of [C ii], far-infrared continuum, optical, and ultraviolet emission. However, a fraction of the sample (∼30 per cent) shows offsets larger than the median by more than 3σ significance (compared to the uncertainty on the offsets), especially between [C ii] and ultraviolet emission. We find that these significant offsets are of the order of ∼0.5–0.7 arcsec, corresponding to ∼3.5–4.5 kiloparsecs. The offsets could be caused by a complex dust geometry, strong feedback from stars and active galactic nuclei, large-scale gas inflow and outflow, or a combination of these phenomena. However, our current analysis does not definitively constrain the origin. Future, higher resolution ALMA and JWST observations may help resolve the ambiguity. Regardless, since there exist at least some galaxies that display such large offsets, galaxy models and spectral energy distribution fitting codes cannot assume co-spatial emission in all main-sequence galaxies, and must take into account that the observed emission across wavelengths may be spatially segregated.
Related Topics
Concepts
Physics
Astrophysics
Galaxy
Submillimeter Array
Stars
Active galactic nucleus
Astronomy
Star formation
Millimeter
Luminous infrared galaxy
Metadata
- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.1093/mnras/stae1371
- https://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stae1371/58036359/stae1371.pdf
- OA Status
- gold
- Cited By
- 8
- References
- 139
- Related Works
- 10
- OpenAlex ID
- https://openalex.org/W4399276678
All OpenAlex metadata
Raw OpenAlex JSON
- OpenAlex ID
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https://openalex.org/W4399276678Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.1093/mnras/stae1371Digital Object Identifier
- Title
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The ALPINE-ALMA [C
ii ] survey: characterization of spatial offsets in main-sequence galaxies at z ∼ 4–6Work title - Type
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articleOpenAlex work type
- Language
-
enPrimary language
- Publication year
-
2024Year of publication
- Publication date
-
2024-05-30Full publication date if available
- Authors
-
Meghana Killi, M. Ginolfi, Gergö Popping, D. Watson, G. Zamorani, B. C. Lemaux, Seiji Fujimoto, Andreas L. Faisst, M. Béthermin, Michael Romano, Yoshinobu Fudamoto, S. Bardelli, M. Boquien, Stefano Carniani, M. Dessauges‐Zavadsky, C. Gruppioni, Nimish P. Hathi, E. Ibar, Gareth C. Jones, Anton M. Koekemoer, Ivanna Langan, Hugo Méndez-Hernández, Yuma Sugahara, L. Vallini, D. VerganiList of authors in order
- Landing page
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https://doi.org/10.1093/mnras/stae1371Publisher landing page
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https://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stae1371/58036359/stae1371.pdfDirect link to full text PDF
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YesWhether a free full text is available
- OA status
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goldOpen access status per OpenAlex
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https://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stae1371/58036359/stae1371.pdfDirect OA link when available
- Concepts
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Physics, Astrophysics, Galaxy, Submillimeter Array, Stars, Active galactic nucleus, Astronomy, Star formation, Millimeter, Luminous infrared galaxyTop concepts (fields/topics) attached by OpenAlex
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8Total citation count in OpenAlex
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2025: 6, 2024: 2Per-year citation counts (last 5 years)
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139Number of works referenced by this work
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10Other works algorithmically related by OpenAlex
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