APA(7版)引用形式

Tatum, M., Turner, T., Sim, S., Miller, L., Reeves, J., Patrick, A., & Long, K. (2012). MODELING THE Fe K LINE PROFILES IN TYPE I ACTIVE GALACTIC NUCLEI WITH A COMPTON-THICK DISK WIND. Institute of Physics Publishing.

Chicagoスタイル(17版)引用形式

Tatum, M., T. Turner, SA Sim, L. Miller, J. Reeves, A. Patrick, , K. Long. MODELING THE Fe K LINE PROFILES IN TYPE I ACTIVE GALACTIC NUCLEI WITH A COMPTON-THICK DISK WIND. Institute of Physics Publishing, 2012.

MLA(9版)引用形式

Tatum, M., et al. MODELING THE Fe K LINE PROFILES IN TYPE I ACTIVE GALACTIC NUCLEI WITH A COMPTON-THICK DISK WIND. Institute of Physics Publishing, 2012.

警告: この引用は必ずしも正確ではありません.