Metha, B., Trenti, M., & Norman, C. (2026). The "bubbly" interstellar medium as origin for the inhomogeneous internal metallicity distributions in large disk galaxies.
Chicago-Zitierstil (17. Ausg.)Metha, Benjamin, Michele Trenti, und Colin Norman. The "Bubbly" Interstellar Medium as Origin for the Inhomogeneous Internal Metallicity Distributions in Large Disk Galaxies. 2026.
MLA-Zitierstil (9. Ausg.)Metha, Benjamin, et al. The "Bubbly" Interstellar Medium as Origin for the Inhomogeneous Internal Metallicity Distributions in Large Disk Galaxies. 2026.
Achtung: Diese Zitate sind unter Umständen nicht zu 100% korrekt.