The research group led by Rie Miura, a graduate student at the University of Tokyo has found evidences of sequential star formation induced by the expansion of a super-giant HII region. The group observed the super-giant HII region called NGC 604 in the Triangulum Galaxy (also known as Messier 33) with the millimeter interferometer of the Nobeyama Radio Astronomical Observatory, and discovered that the star formation activity decreases with increasing projected distance from the central cluster. This is the first time to unveil the process of sequential star formation in a giant extragalactic HII region. The group is going to investigate star formation in the giant HII region with ALMA that allows celestial observations at much higher resolution and sensitivity. Please visit http://alma.mtk.nao.ac.jp/~miura/index-e.html for more detailed information.
NEW ARTICLES
2025 6.26
Development of Total Power GPU Spectrometer was approved by ALMA Board
In April 2025, the ALMA Board approved the development of a new spectrometer for the Morita Array (*) designed and deve…
2025 6.24
New Super-resolution Imaging Reveals the First Step of Planet Formation after Star Birth
A research team led by Ayumu Shoshi of Kyushu University and the Academia Sinica Institute of Astronomy and Astrophysic…
2025 6.3
Joint ALMA Observatory Open Day 2025
- Tags
- News ALMA Topics Events
On March 21, 2025, NAOJ participated in the public event "Open Day 2025" held at the Joint ALMA Observatory in Santiago…