Hostname: page-component-848d4c4894-nmvwc Total loading time: 0 Render date: 2024-06-26T17:25:21.915Z Has data issue: false hasContentIssue false

The nature of the Galactic bulge: A view from bulge planetary nebulae and globular clusters

Published online by Cambridge University Press:  30 August 2012

Alexander F. Kholtygin
Affiliation:
Sobolev Astronomical Institute, Saint Petersburg State University, Universitetskij pr. 28, Staryj Peterhof, Saint Petersburg 198504, Russia email: afkholtygin@gmail.com
Yulia V. Milanova
Affiliation:
Sobolev Astronomical Institute, Saint Petersburg State University, Universitetskij pr. 28, Staryj Peterhof, Saint Petersburg 198504, Russia email: afkholtygin@gmail.com
Igor' I. Nikiforov
Affiliation:
Sobolev Astronomical Institute, Saint Petersburg State University, Universitetskij pr. 28, Staryj Peterhof, Saint Petersburg 198504, Russia email: afkholtygin@gmail.com
Olga V. Vasyakina
Affiliation:
Sobolev Astronomical Institute, Saint Petersburg State University, Universitetskij pr. 28, Staryj Peterhof, Saint Petersburg 198504, Russia email: afkholtygin@gmail.com
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.

Modern data concerning the planetary nebulae (PNe) in the bulge, bar and disk of the Milky Way are used to study the chemical history of bulge. We show that the abundance pattern is similar for PNe in the bulge and Peimbert's type II PNe. We also found that the globular clusters (GCs), especially their metal-rich disk subsystem, form on metallicity maps a bar-like structure which parameters are very close to those for the Galactic bar. These results evidence an old age of the Galactic bulge and bar. We propose a scenario of the successive star formation in the bulge, bar and thin disk.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2012

References

Akimkin, V. V., Nikiforov, I. I., & Kholtygin, A. F. MNRAS, in preparationGoogle Scholar
Gardner, E. & Flynn, C. 2010, MNRAS, 405, 545 Google Scholar
Harris, W. E. 1996, AJ 112 1487; arXiv:1012.3224 (2010 edition)CrossRefGoogle Scholar
Immeli, A., Samland, M., & Gerhard, O. 2004, A&A, 413, 547 Google Scholar
Milanova, Yu. V. & Kholtygin, A. F. 2009, Astron. Lett., 35, 518 CrossRefGoogle Scholar
Quireza, C., Rocha-Pinto, H. J., & Maciel, W. J. 2007, A&A, 475, 217 Google Scholar