American Psychological Association 6th edition

ANTOKHIN, I. I., OWOCKI, S. P., & BROWN, J. C. (2004). A steady, radiative-shock method for computing X-ray emission from colliding stellar winds in close, massive-star binaries. The Astrophysical Journal, 611(1), 434-451.

ISO-690 (author-date, English)

ANTOKHIN, I. I, OWOCKI, S. P and BROWN, J. C, 2004. A steady, radiative-shock method for computing X-ray emission from colliding stellar winds in close, massive-star binaries. The Astrophysical journal. 1 January 2004. Vol. 611, no. 1, p. 434-451.

Modern Language Association 9th edition

ANTOKHIN, I. I., S. P. OWOCKI, and J. C. BROWN. “A Steady, Radiative-Shock Method for Computing X-Ray Emission from Colliding Stellar Winds in Close, Massive-Star Binaries”. The Astrophysical Journal, vol. 611, no. 1, Jan. 2004, pp. 434-51.

Mohr Siebeck - Recht (Deutsch - Österreich)

ANTOKHIN, I. I/OWOCKI, S. P/BROWN, J. C: A steady, radiative-shock method for computing X-ray emission from colliding stellar winds in close, massive-star binaries, The Astrophysical journal 2004, 434-451.

Emerald - Harvard

ANTOKHIN, I.I., OWOCKI, S.P. and BROWN, J.C. (2004), “A steady, radiative-shock method for computing X-ray emission from colliding stellar winds in close, massive-star binaries”, The Astrophysical Journal, Vol. 611 No. 1, pp. 434-451.

Warning: These citations may not always be 100% accurate.