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Gas around galaxy haloes: methodology comparisons using hydrodynamical simulations of the intergalactic medium

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Gas around galaxy haloes: methodology comparisons using hydrodynamical simulations of the intergalactic medium. / Meiksin, Avery; Bolton, James S.; Tittley, Eric R.

In: Monthly Notices of the Royal Astronomical Society, Vol. 445, No. 3, 11.12.2014, p. 2462-2475.

Research output: Contribution to journalArticle

Harvard

Meiksin, A, Bolton, JS & Tittley, ER 2014, 'Gas around galaxy haloes: methodology comparisons using hydrodynamical simulations of the intergalactic medium' Monthly Notices of the Royal Astronomical Society, vol. 445, no. 3, pp. 2462-2475. DOI: 10.1093/mnras/stu1938

APA

Meiksin, A., Bolton, J. S., & Tittley, E. R. (2014). Gas around galaxy haloes: methodology comparisons using hydrodynamical simulations of the intergalactic medium. Monthly Notices of the Royal Astronomical Society, 445(3), 2462-2475. DOI: 10.1093/mnras/stu1938

Vancouver

Meiksin A, Bolton JS, Tittley ER. Gas around galaxy haloes: methodology comparisons using hydrodynamical simulations of the intergalactic medium. Monthly Notices of the Royal Astronomical Society. 2014 Dec 11;445(3):2462-2475. Available from, DOI: 10.1093/mnras/stu1938

Author

Meiksin, Avery ; Bolton, James S. ; Tittley, Eric R./ Gas around galaxy haloes: methodology comparisons using hydrodynamical simulations of the intergalactic medium. In: Monthly Notices of the Royal Astronomical Society. 2014 ; Vol. 445, No. 3. pp. 2462-2475