APA (7th ed.) Citation

Bartalucci, I., Arnaud, M., Pratt, G., & Le Brun, A. M. C. (2018). Resolving the hydrostatic mass profiles of galaxy clusters at z ∼ 1 with XMM-Newton and Chandra. Astronomy & Astrophysics / Astronomie et Astrophysique, 617, N.PAG. https://doi.org/10.1051/0004-6361/201732458

Chicago Style (17th ed.) Citation

Bartalucci, I., M. Arnaud, G.W Pratt, and A. M. C. Le Brun. "Resolving the Hydrostatic Mass Profiles of Galaxy Clusters at Z ∼ 1 with XMM-Newton and Chandra." Astronomy & Astrophysics / Astronomie Et Astrophysique 617 (2018): N.PAG. https://doi.org/10.1051/0004-6361/201732458.

MLA (8th ed.) Citation

Bartalucci, I., et al. "Resolving the Hydrostatic Mass Profiles of Galaxy Clusters at Z ∼ 1 with XMM-Newton and Chandra." Astronomy & Astrophysics / Astronomie Et Astrophysique, vol. 617, 2018, p. N.PAG, https://doi.org/10.1051/0004-6361/201732458.

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