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Search for binary central stars of the Magellanic Clouds PNe

Published online by Cambridge University Press:  08 August 2017

Marcin Gładkowski ,
Marcin Hajduk  and
Igor Soszyński
Marcin Gładkowski
Affiliation:
Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, ul. Rabiańska 8, 87-100 Toruń, Poland email: seyfert@ncac.torun.pl
Marcin Hajduk
Affiliation:
National Science Centre, ul. Królewska 57, 30-081 Kraków, Poland
Igor Soszyński
Affiliation:
Obserwatorium Astronomiczne, Uniwersytet Warszawski, Al. Ujazdowskie 4, 00-478, Warszawa, Poland
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Abstract

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The Optical Gravitational Experiment (OGLE) was effectively used in discovering binary central stars of planetary nebulae (CSPNe). About 50 binary CSPNe have been hitherto identified in the Galaxy, almost half of them were detected in the OGLE database. We used the OGLE data to search for binary CSPNe in the Magellanic Clouds. We also searched for PNe mimics and removed them from the PNe sample. Here, we present results of the photometric analysis for Small Magellanic Cloud (SMC) and our progress on search of binary central stars in the Large Magellanic Cloud (LMC). So far, we have discovered one binary central star of the PN beyond the Milky Way, which is located in the Small Magellanic Cloud.

Keywords

techniques: photometricbinaries: generalplanetary nebulae: generalMagellanic Clouds
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S323: Planetary Nebulae: Multi-Wavelength Probes of Stellar and Galactic Evolution , October 2016 , pp. 384 - 385
Copyright
Copyright © International Astronomical Union 2017 

References

Boffin, H. M. J., Miszalski, B., Rauch, T., et al. 2012, Science, 338, 773 Google Scholar
Bond, H. E., 2000, ASP Conf. Ser., 199, 115 Google Scholar
De Marco, O., 2009, PASP, 121, 316 CrossRefGoogle Scholar
Hajduk, M., Gładkowski, M., & Soszyński, I., 2014, A&A, 561, A8 Google Scholar
Haberl, F. & Sasaki, M., 2000, A&A, 359, 573 Google Scholar
Hajduk, M., Gromadzki, M., Mikołajewska, J., Miszalski, B., & Soszyński, I. 2015, Acta Astronomica, 65, no 2, 139-149 Google Scholar
Lenz, P. & Breger, M., 2005, Comm. Asteroseismol., 146, 53 CrossRefGoogle Scholar
Miszalski, B., Acker, A., Moffat, A. F. J., Parker, Q. A., & Udalski, A., 2009, A&A, 496, 813-825 Google Scholar
Miszalski, B., Acker, A., Parker, Q. A., & Moffat, A. F. J., 2009, A&A, 505, 249 Google Scholar
Schwarzenberg-Czerny, A., 1996, ApJ, 460, L107 Google Scholar