RAMBO. I. Project Introduction and First Results with uGMRT Article Swipe
YOU?
·
· 2025
· Open Access
·
· DOI: https://doi.org/10.3847/1538-4357/adbbba
Magnetic hot stars can emit both coherent and incoherent nonthermal radio emission. Understanding the nature of these emissions and their connection to stellar rotation and magnetic field characteristics remains incomplete. The RAdio Magnetospheres of B and O stars (RAMBO) project aims to address this gap by systematically detecting and characterizing gyrosynchrotron and cyclotron maser radio emission in rapidly rotating magnetic hot stars. Using the upgraded Giant Metrewave Radio Telescope, we present the first detection of radio emission from HD 55522 at 650 MHz, confirming it as a new radio-bright magnetic hot star. This supports the predictions of the Centrifugal Breakout model, furthering its application in understanding particle acceleration mechanisms in centrifugal magnetospheres of hot stars. Additionally, we report nondetections for four other targets, improving sensitivity limits by a factor of a few compared to previous observations. These findings demonstrate the potential of RAMBO to uncover the complexities of radio emission in massive stars and highlight the need for broader, multiwavelength observations to probe magnetospheric physics comprehensively. The sensitivity of the Square Kilometre Array will enable significant advancements.
Related Topics
- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.3847/1538-4357/adbbba
- OA Status
- gold
- References
- 103
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- OpenAlex ID
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Raw OpenAlex JSON
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https://openalex.org/W4409070209Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.3847/1538-4357/adbbbaDigital Object Identifier
- Title
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RAMBO. I. Project Introduction and First Results with uGMRTWork title
- Type
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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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2025-04-01Full publication date if available
- Authors
-
Z. Keszthelyi, Kohei Kurahara, Yuhei Iwata, Yuka Fujii, Haruka Sakemi, Koh Takahashi, Shintaro YoshiuraList of authors in order
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https://doi.org/10.3847/1538-4357/adbbbaPublisher landing page
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YesWhether a free full text is available
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goldOpen access status per OpenAlex
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https://doi.org/10.3847/1538-4357/adbbbaDirect OA link when available
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Physics, Astronomy, AstrophysicsTop concepts (fields/topics) attached by OpenAlex
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0Total citation count in OpenAlex
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103Number of works referenced by this work
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10Other works algorithmically related by OpenAlex
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| abstract_inverted_index.demonstrate | 139 |
| abstract_inverted_index.incomplete. | 30 |
| abstract_inverted_index.predictions | 96 |
| abstract_inverted_index.sensitivity | 125, 168 |
| abstract_inverted_index.significant | 176 |
| abstract_inverted_index.acceleration | 108 |
| abstract_inverted_index.complexities | 147 |
| abstract_inverted_index.observations | 161 |
| abstract_inverted_index.radio-bright | 89 |
| abstract_inverted_index.Additionally, | 116 |
| abstract_inverted_index.Understanding | 13 |
| abstract_inverted_index.advancements. | 177 |
| abstract_inverted_index.nondetections | 119 |
| abstract_inverted_index.observations. | 136 |
| abstract_inverted_index.understanding | 106 |
| abstract_inverted_index.Magnetospheres | 33 |
| abstract_inverted_index.characterizing | 50 |
| abstract_inverted_index.magnetospheres | 112 |
| abstract_inverted_index.magnetospheric | 164 |
| abstract_inverted_index.systematically | 47 |
| abstract_inverted_index.characteristics | 28 |
| abstract_inverted_index.gyrosynchrotron | 51 |
| abstract_inverted_index.multiwavelength | 160 |
| abstract_inverted_index.comprehensively. | 166 |
| cited_by_percentile_year | |
| countries_distinct_count | 0 |
| institutions_distinct_count | 7 |
| citation_normalized_percentile.value | 0.08931913 |
| citation_normalized_percentile.is_in_top_1_percent | False |
| citation_normalized_percentile.is_in_top_10_percent | False |