| DOI | Resolve DOI: https://doi.org/10.1051/eas/1571026 |
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| Author | Search for: Hrivnak, B. J.; Search for: Lu, W.; Search for: Van de Steene, G.; Search for: Van Winckel, H.; Search for: Sperauskas, J.; Search for: Bohlender, D.1 |
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| Editor | Search for: Lagadec, E. |
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| Name affiliation | - National Research Council of Canada. National Science Infrastructure
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| Format | Text, Article |
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| Conference | The Physics of Evolved Stars: A Conference Dedicated to the Memory of Olivier Chesneau, June 8–12, 2015, Nice, France |
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| Abstract | We have investigated pulsations and searched for binarity in 7 bright proto-planetary nebulae. All are found to pulsate, with dominant periods of 39−132 days. However, no strong evidence of binarity is found in any of them. This implies that any binary companion must have either a very long period (>30 yr) or low mass (<0.2 Msun). This appears to rule out Roche lobe overflow as a contribution to the shaping of the surrounding nebula. |
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| Publication date | 2015-12-01 |
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| Language | English |
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| Peer reviewed | Yes |
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| Identifier | eas1571026 |
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| NPARC number | 23000659 |
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| Export citation | Export as RIS |
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| Report a correction | Report a correction (opens in a new tab) |
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| Record identifier | 1a0c57e8-e602-4b84-84cb-d89f1f9cf10d |
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| Record created | 2016-08-18 |
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| Record modified | 2020-04-22 |
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