Bik, A., Henning, T., & Pasquali, A. (2019). Near-infrared spectroscopy of the massive stellar population of W51: Evidence for multi-seeded star formation. Astronomy and astrophysics, 624, . https://doi.org/10.1051/0004-6361/201935061
Chicago-Zitierstil (17. Ausg.)Bik, Arjan, Thomas Henning, und Anna Pasquali. "Near-infrared Spectroscopy of the Massive Stellar Population of W51: Evidence for Multi-seeded Star Formation." Astronomy and Astrophysics 624 (2019). https://doi.org/10.1051/0004-6361/201935061.
MLA-Zitierstil (9. Ausg.)Bik, Arjan, et al. "Near-infrared Spectroscopy of the Massive Stellar Population of W51: Evidence for Multi-seeded Star Formation." Astronomy and Astrophysics, vol. 624, 2019, https://doi.org/10.1051/0004-6361/201935061.
Achtung: Diese Zitate sind unter Umständen nicht zu 100% korrekt.