Hostname: page-component-8448b6f56d-42gr6 Total loading time: 0 Render date: 2024-04-24T22:03:49.971Z Has data issue: false hasContentIssue false

Helium abundances in inner Galaxy planetary nebulae

Published online by Cambridge University Press:  23 April 2010

Oscar Cavichia
Affiliation:
IAG, University of São Paulo, 05508-900, São Paulo-SP, Brazil email: cavichia@astro.iag.usp.br
Roberto D. D. Costa
Affiliation:
IAG, University of São Paulo, 05508-900, São Paulo-SP, Brazil
Walter J. Maciel
Affiliation:
IAG, University of São Paulo, 05508-900, São Paulo-SP, Brazil
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

New helium abundances of planetary nebulae located towards the bulge of the Galaxy were derived, based on observations made at OPD (Brazil). We present accurate helium abundances for 56 PNe located towards the galactic bulge. The data show good agreement with other results in the literature, in the sense that the distribution of the abundances is similar to previous works. Furthermore, the radial helium gradient is extended towards the galactic center. The results show that no trend can be identified when comparing the internal gradient (R ≤ 4 kpc) to the whole galactic disk.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2010

References

Cavichia, O., Costa, R. D. D., & Maciel, W. J. 2009, Rev. Mexicana AyA, (Submitted)Google Scholar
Chiappini, C., Matteucci, F., & Romano, D. 2001, ApJ, 554, 1044CrossRefGoogle Scholar
Costa, R. D. D., Uchida, M. M. M., & Maciel, W. J. 2004, A&A, 423, 199Google Scholar
Costa, R. D. D., Maciel, W. J., & Escudero, A. V. 2008, Baltic Astronomy, 17, 321Google Scholar
Escudero, A. V., Costa, R. D. D., & Maciel, W. J. 2004, A&A, 414, 211Google Scholar
Maciel, W. J. 2000, in: da Silva, L., de Medeiros, R., & Spite, M. (eds.), The Light Elements and their Evolution, Proc. IAU Symposium No. 198, p. 204Google Scholar
Stanghellini, L., Shaw, R. A., & Villaver, E. 2008, ApJ, 689, 194CrossRefGoogle Scholar