Oxygen abundance in giant H II galaxies-Reference-Cited by-同舟云学术

Oxygen abundance in giant H II galaxies

Published:2010-10 Issue:5 Volume:26 Page:215-232
ISSN:0884-5913
Container-title:Kinematics and Physics of Celestial Bodies
language:en
Short-container-title:Kinemat. Phys. Celest. Bodies

Author:

Pilyugin L. S.,Zinchenko I. A.,Thuan T. X.

Publisher

Allerton Press

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.3103/S0884591310050016.pdf

Reference48 articles.

1. C. W. Allen, Astrophysical Quantities, 3rd ed. (Mir, Moscow, 1977; Athlone Press, London, 1973).

2. L. S. Pilyugin, I. Yu. Izotova, and Yu. S. Sholudchenko, “Oxygen Abundance in Nearby Galaxies Based on the Spectra of H II Regions from the Sloan Digital Sky Survey II: The Interacting Galaxies NGC 4631 and NGC 4656,” Kinem. Fiz. Nebes. Tel 24, 263–277 (2008) [Kinem. Phys. Celest. Bodies 24, 192 (2008)].

3. Yu. S. Sholudchenko, I. Yu. Izotova, and L. S. Pilyugin, “The Oxygen Abundance in the H II Regions of the Spiral Galaxy M101 Determined from the Sloan Digital Sky Survey Spectra,” Kinem. Fiz. Nebes. Tel 23, 230–240 (2007) [Kinem. Phys. Celest. Bodies 23, 163 (2007)].

4. K. M. Aggarwal and F. P. Keenan, “Excitation Rate Coefficients for Fine-Structure Transitions in OIII,” Astrophys. J., Suppl. Ser. 123, 311–349 (1999).

5. B. Argence and F. Lamareille, “Emission-Lines Calibrations of the Formation Rate from the Sloan Digital Sky Survey,” Astron. Astrophys. 495, 759–773 (2009).

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