An accreting pulsar with extreme properties drives an ultraluminous x-ray source in NGC 5907.

MLA

Luca Israel, Gian, et al. “An Accreting Pulsar with Extreme Properties Drives an Ultraluminous X-Ray Source in NGC 5907.” Science, vol. 355, no. 6327, Feb. 2017, pp. 817–19. EBSCOhost, https://doi.org/10.1126/science.aai8635.

APA

Luca Israel, G., Belfiore, A., Stella, L., Esposito, P., Casella, P., De Luca, A., Marelli, M., Papitto, A., Perri, M., Puccetti, S., Rodríguez Castillo, G. A., Salvetti, D., Tiengo, A., Zampieri, L., D, A. D., Greiner, J., Haberl, F., Novara, G., Salvaterra, R., & Turolla, R. (2017). An accreting pulsar with extreme properties drives an ultraluminous x-ray source in NGC 5907. Science, 355(6327), 817–819. https://doi.org/10.1126/science.aai8635

Chicago

Luca Israel, Gian, Andrea Belfiore, Luigi Stella, Paolo Esposito, Piergiorgio Casella, Andrea De Luca, Martino Marelli, et al. 2017. “An Accreting Pulsar with Extreme Properties Drives an Ultraluminous X-Ray Source in NGC 5907.” Science 355 (6327): 817–19. doi:10.1126/science.aai8635.