The young massive SMC cluster NGC 330 seen by MUSE. II. Multiplicity properties of the massive-star population

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SEEK ID: https://publications.h-its.org/publications/1309

SEEK ID: https://publications.h-its.org/publications/1309

DOI: 10.1051/0004-6361/202140507

Research Groups: Stellar Evolution Theory

Publication type: Journal

Journal: Astronomy and Astrophysics

Citation: A&A 652:A70

Date Published: 1st Aug 2021

Registered Mode: imported from a bibtex file

Authors: J. Bodensteiner, H. Sana, C. Wang, N. Langer, L. Mahy, G. Banyard, A. de Koter, S. E. de Mink, C. J. Evans, Y. Götberg, L. R. Patrick, F. R. N. Schneider, F. Tramper

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Bodensteiner, J., Sana, H., Wang, C., Langer, N., Mahy, L., Banyard, G., de Koter, A., de Mink, S. E., Evans, C. J., Götberg, Y., Patrick, L. R., Schneider, F. R. N., & Tramper, F. (2021). The young massive SMC cluster NGC 330 seen by MUSE. In Astronomy & Astrophysics (Vol. 652, p. A70). EDP Sciences. https://doi.org/10.1051/0004-6361/202140507
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Created: 11th Nov 2021 at 22:40

Last updated: 5th Mar 2024 at 21:24

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