Tamura, Yoichi
Tamura is a co-author of the study 'Bound star clusters observed in a lensed galaxy 460 Myr after the Big Bang', published in Nature. The research focuses on observing five star clusters located in a region smaller than 70 parsec of an intrinsically UV faint galaxy, which is thought to drive the reionization of the universe. Despite uncertainties inherent to the lensing model, these star clusters exhibit minimal dust attenuation and low metallicity, ages younger than 50 Myr and intrinsic masses of less than 106 M₎. Their lensing-corrected sizes are approximately 1 pc, resulting in stellar surface densities near 105 M₎/pc2. The authors conclude that star cluster formation and feedback likely contributed to shaping the properties of galaxies during the epoch of reionization.
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The Daily's Verdict
This author is known for its high journalistic standards. The author strives to maintain neutrality and transparency in its reporting, and avoids conflicts of interest. The author has a reputation for accuracy and rarely gets contradicted on major discrepancies in its reporting.
Bias
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No current examples available.
Conflicts of Interest
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No current examples available.
Contradictions
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Examples:
- The authors suggest that these star clusters are gravitationally bound stellar systems, i.e., proto-globular clusters (proto-GCs). Yet, they acknowledge that there are uncertainties inherent to the lensing model.
- The author states that the galaxy is intrinsically UV faint and in the range of those now thought to drive the reionization of the universe. However, they also report observing five star clusters with minimal dust attenuation and low metallicity.
Deceptions
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No current examples available.
Recent Articles
New Discovery of Five Young Star Clusters in Infant Galaxy Reveals Insights into Star Formation during the Epoch of Reionization
Broke On: Saturday, 22 June 2024Astronomers discovered five young star clusters in the Cosmic Gems arc, a strongly-lensed galaxy from the reionization era. These clusters, exhibiting minimal dust attenuation and low metallicity, offer insights into star formation during this epoch. Gravitational lensing revealed details of infant galaxies and their globular cluster formation.