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ALMAGAL

Context. The fragmentation of massive molecular clumps into smaller, potentially star-forming cores plays a key role in the processes of high-mass star formation. The ALMAGAL project, using the Atacama Large Millimeter/submillimeter Array (ALMA), offers highr-esolution data to investigate these proc...

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Principais autores: Elia D., Coletta A., Molinari S., Schisano E., Benedettini M., Sánchez-Monge Á., Traficante A., Mininni C., Nucara A., Pezzuto S., Schilke P., Soler J. D., Avison A., Beltrán M. T., Beuther H., Clarke S., Fuller G. A., Klessen R. S., Kuiper R., Lebreuilly U., Lis D. C., Möller T., Moscadelli L., Rigby A. J., Sanhueza P., van der Tak F., Zhang Q., Rygl K. L. J., Merello M., Battersby C., Ho P. T. P., Klaassen P. D., Koch P. M., Allande J., Bronfman L., Fontani F., Hennebelle P., Jones B., Liu T., Stroud G., Wells M. R. A., Ahmadi A., Brogan C. L., De Angelis F., Hunter T. R., Johnston K. G., Law C. Y., Liu S. J., Liu S.-Y., Maruccia Y., Pelkonen V.-M., Su Y.-N., Tang Y., Testi L., Walch S., Zhang T., Zinnecker H.
Format: Artigo
Jezik:Inglês
Izdano: EDP Sciences 2026-01-01
Serija:Astronomy & Astrophysics
Teme:
methods: observational
techniques: interferometric
stars: formation
ism: clouds
ism: structure
submillimeter: ism
Online dostop:https://www.aanda.org/articles/aa/full_html/2026/01/aa54764-25/aa54764-25.html
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