Cite
The anomalous polymict ordinary chondrite breccia of Elmshorn (H3‐6)—Late reaccretion after collision between two ordinary chondrite parent bodies, complete disruption, and mixing possibly about 2.8 Gyr ago.
MLA
Bischoff, Addi, et al. “The Anomalous Polymict Ordinary Chondrite Breccia of Elmshorn (H3‐6)—Late Reaccretion after Collision between Two Ordinary Chondrite Parent Bodies, Complete Disruption, and Mixing Possibly about 2.8 Gyr Ago.” Meteoritics & Planetary Science, May 2024, p. 1. EBSCOhost, https://doi.org/10.1111/maps.14193.
APA
Bischoff, A., Patzek, M., Alosius, R. M. L., Barrat, J., Berndt, J., Busemann, H., Degering, D., Di Rocco, T., Ek, M., Gattacceca, J., Godinho, J. R. A., Heinlein, D., Krietsch, D., Maden, C., Marchhart, O., Martschini, M., Merchel, S., Pack, A., Peters, S., & Rüfenacht, M. (2024). The anomalous polymict ordinary chondrite breccia of Elmshorn (H3‐6)—Late reaccretion after collision between two ordinary chondrite parent bodies, complete disruption, and mixing possibly about 2.8 Gyr ago. Meteoritics & Planetary Science, 1. https://doi.org/10.1111/maps.14193
Chicago
Bischoff, Addi, Markus Patzek, Romain M. L. Alosius, Jean‐Alix Barrat, Jasper Berndt, Henner Busemann, Detlev Degering, et al. 2024. “The Anomalous Polymict Ordinary Chondrite Breccia of Elmshorn (H3‐6)—Late Reaccretion after Collision between Two Ordinary Chondrite Parent Bodies, Complete Disruption, and Mixing Possibly about 2.8 Gyr Ago.” Meteoritics & Planetary Science, May, 1. doi:10.1111/maps.14193.