The central parsec of NGC 3783: a rotating broad emission line region, asymmetric hot dust structure, and compact coronal line region

MLA

GRAVITY Collaboration, et al. The Central Parsec of NGC 3783: A Rotating Broad Emission Line Region, Asymmetric Hot Dust Structure, and Compact Coronal Line Region. 2021. EBSCOhost, https://doi.org/10.1051/0004-6361/202040061.

APA

GRAVITY Collaboration, Amorim, A., Bauböck, M., Brandner, W., Bolzer, M., Clénet, Y., Davies, R., de Zeeuw, P. T., Dexter, J., Drescher, A., Eckart, A., Eisenhauer, F., Schreiber, N. M. F., Gao, F., Garcia, P. J. V., Genzel, R., Gillessen, S., Gratadour, D., Hönig, S., … Woillez, J. (2021). The central parsec of NGC 3783: a rotating broad emission line region, asymmetric hot dust structure, and compact coronal line region. https://doi.org/10.1051/0004-6361/202040061

Chicago

GRAVITY Collaboration, A. Amorim, M. Bauböck, W. Brandner, M. Bolzer, Y. Clénet, R. Davies, et al. 2021. “The Central Parsec of NGC 3783: A Rotating Broad Emission Line Region, Asymmetric Hot Dust Structure, and Compact Coronal Line Region.” doi:10.1051/0004-6361/202040061.