Jetted subgalactic-size radio sources in merging galaxies Article Swipe
YOU?
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· 2025
· Open Access
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· DOI: https://doi.org/10.1051/0004-6361/202451334
Context. The long-standing question concerning jetted subgalactic-size (JSS) radio sources is whether they will evolve into large radio galaxies, die before escaping the host galaxy, or remain indefinitely confined to their compact size. Aims. Our main goal is to propose a scenario that explains the relative number of JSS radio sources and their general properties. Methods. We studied the parsec-scale radio morphology of a complete sample of 21 objects using Very Long Baseline Array (VLBA) observations at various frequencies and analyzed the morphological characteristics of their optical hosts. Results. Many of these radio sources exhibit radio morphologies consistent with transverse motions of their bright edges and are found in dynamically disturbed galaxies. VLBA images suggest the possible presence of large-angle, short-period precessing jets, and an orbital motion of the radio-loud active galactic nucleus (AGN) in a dual or binary system. The majority of JSS radio sources appear to be in systems in different stages of their merging evolution. Conclusions. We propose a scenario where rapid jet redirection, through precession or orbital motion, prevents the jet from penetrating the interstellar medium (ISM) sufficiently to escape the host galaxy. Most JSS radio sources remain compact due to their occurrence in merging galaxies.
Related Topics
- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.1051/0004-6361/202451334
- OA Status
- hybrid
- Cited By
- 3
- References
- 92
- Related Works
- 10
- OpenAlex ID
- https://openalex.org/W4407788508
Raw OpenAlex JSON
- OpenAlex ID
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https://openalex.org/W4407788508Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.1051/0004-6361/202451334Digital Object Identifier
- Title
-
Jetted subgalactic-size radio sources in merging galaxiesWork title
- Type
-
articleOpenAlex work type
- Language
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enPrimary language
- Publication year
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2025Year of publication
- Publication date
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2025-02-20Full publication date if available
- Authors
-
C. Stanghellini, M. Orienti, Cristiana Spingola, A. Zanichelli, D. Dallacasa, P. Cassaro, C.P. O'Dea, Sebastian Baum, M-A. Perez-TorresList of authors in order
- Landing page
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https://doi.org/10.1051/0004-6361/202451334Publisher landing page
- Open access
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YesWhether a free full text is available
- OA status
-
hybridOpen access status per OpenAlex
- OA URL
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https://doi.org/10.1051/0004-6361/202451334Direct OA link when available
- Concepts
-
Physics, Astrophysics, Radio galaxy, X-shaped radio galaxy, Galaxy, Jet (fluid), Astronomy, Astrophysical jet, Active galactic nucleus, ThermodynamicsTop concepts (fields/topics) attached by OpenAlex
- Cited by
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3Total citation count in OpenAlex
- Citations by year (recent)
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2025: 3Per-year citation counts (last 5 years)
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92Number of works referenced by this work
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10Other works algorithmically related by OpenAlex
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| abstract_inverted_index.a | 40, 63, 135, 161 |
| abstract_inverted_index.21 | 67 |
| abstract_inverted_index.We | 56, 159 |
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| abstract_inverted_index.is | 10, 37 |
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| abstract_inverted_index.(ISM) | 180 |
| abstract_inverted_index.(JSS) | 7 |
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| abstract_inverted_index.found | 107 |
| abstract_inverted_index.jets, | 122 |
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| abstract_inverted_index.radio | 8, 17, 49, 60, 92, 95, 144, 189 |
| abstract_inverted_index.rapid | 164 |
| abstract_inverted_index.size. | 32 |
| abstract_inverted_index.their | 30, 52, 85, 102, 155, 195 |
| abstract_inverted_index.these | 91 |
| abstract_inverted_index.using | 69 |
| abstract_inverted_index.where | 163 |
| abstract_inverted_index.(VLBA) | 74 |
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| abstract_inverted_index.before | 20 |
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| abstract_inverted_index.compact | 31, 192 |
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| abstract_inverted_index.galaxy. | 186 |
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