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Volume 1, Issue 1 (2019) , Pages [1] - [182]
TEMPERATURE STRUCTURE OF METAL ENRICHED NOVAE
[1] H. K. B. Beck, P. H. Hauschildt, H. P. Gali and
[2] P. B. Bosma, the state of ionization in novae shell, A&A 40 (1975), 175.
[3] A. Dalgarno and S. Lepp, Atomic, Molecular and Optical Physics Handbook, Edited by Drake G., W., F., AIP Press, New York, 1996.
[4] C. Esteban, M. Peimbert, J. Garcia-Rojas, M. T. Ruiz, A. Peimbert and M. Rodriguez, 2004, Carbon and oxygen galactic gradients I: Observational values from H II region recombination lines, MNRAS 335 (1998), 229.
[5] G. J. Ferland et al., Hazy: Introduction to Cloudy c13.03, 2013.
[6] J. P. Harrington, Ionization stratification and chemical abundances in the planetary nebulae, Astrophys. J. 156 (1969), 903.
[7] G. M. MacAlpine, Photoionization model for the emission line regions of quasi-stellar and related objects, ApJ 175 (1972), 11.
[8] S. S. McGaugh, H II region abundances: Model oxygen line ratios, ApJ 380 (1991), 140.
[9] D. E. Osterbrock, Astrophysics of Gaseous Nebulae and Active Galactic Nuclei,
[10] D. E. Osterbrock and G. J. Ferland, Astrophysics of Gaseous Nebulae and Active Galactic Nuclei, 2nd Edition, University Science Books, 2005.
[11] M. Peimbert, Temperature determinations of H II regions, ApJ 150 (1967), 825.
[12] M. Peimbert, In the Analysis of Emission Lines, Proceedings of the Space Telescope Science Institute Symposium Number 8, Editors R. Williams & M. Livio (Cambridge CUP), 165, 1995.
[13] M. Pontefract and J. M. C. Rawlings, The early chemical evolution of nova outflows, MNRAS 347 (2004), 1294.
[14] P. C. Robert, R. P. C. Wiersma, J. Joop Schaye, D. Britton and B. D. Smith, 2008, arXiv:0807.3748v2 [astro-ph].
[15] G. J. Schwarz, S. Starrfield, S. N. Shore and P. H. Hauschildt, Abundance analysis of the slow nova PW Vulpeculae 1984, 1997, arXiv:astro-ph/9705086v1.
[16] L. Searle, Evidence for composition gradients across the disks of spiral galaxies, ApJ 168 (1971), 327.
[17] M. J. Seaton, MNRAS 189 (1968), 129.
[18] A. M. Serenellil, S. Basu, J. W. Ferguson and M. Asplund, New solar composition: The problems with solar models, ApJ 705 (2009), L123.
[19] D. P. Smith, Photoionization model of metal enriched novae shell, MNRAS 248 (1991), 217.
[20] Y. Zhang, W. Liu, R. Wesson, P. J. Storey, Y. Liu and I. J. Danziger, Electron temperature and densities of planetary nebulae determined from the nebular hydrogen recombination spectrum and electron density, MNRAS 351 (2004), 935