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Post-common-envelope binary central stars of Planetary Nebulae in the OGLE-IV survey
Planetary Nebulae (PNe) are defined as the ionized shells of circumstellar gas ejected through an intense stellar wind at the end of the star's life. PNe come in different shapes, from spherical to highly complex, non-spherical shapes. Mass loss in AGB stars is presumed as the shaping mechanism but...
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| Language: | English |
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Department of Astronomy
2016
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