An Interacting Binary System Powers Precessing Outflows of an Evolved Star
Stars are generally spherical, yet their gaseous envelopes often appear nonspherical when ejected near the end of their lives. This quirk is most notable during the planetary nebula phase, when these envelopes become ionized. Interactions among stars in a binary system are suspected to cause the asy...
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| Published in | Science (American Association for the Advancement of Science) Vol. 338; no. 6108; pp. 773 - 775 |
|---|---|
| Main Authors | , , , , , , , |
| Format | Journal Article |
| Language | English |
| Published |
Washington, DC
American Association for the Advancement of Science
09.11.2012
The American Association for the Advancement of Science |
| Subjects | |
| Online Access | Get full text |
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| Abstract | Stars are generally spherical, yet their gaseous envelopes often appear nonspherical when ejected near the end of their lives. This quirk is most notable during the planetary nebula phase, when these envelopes become ionized. Interactions among stars in a binary system are suspected to cause the asymmetry. In particular, a precessing accretion disk around a companion is believed to launch point-symmetric jets, as seen in the prototype Fleming 1. Our finding of a post-common-envelope binary nucleus in Fleming 1 confirms that this scenario is highly favorable. Similar binary interactions are therefore likely to explain these kinds of outflows in a large variety of systems. |
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| AbstractList | Planetary nebulae form toward the end of the lives of sunlike stars. They appear after the star has shed its outer layers, and radiation from what is left of it ionizes the surrounding medium. Using the Very Large Telescope in Chile, Boffin et al. (p. 773) obtained spectra of the star at the center of Fleming 1, a point-symmetric planetary nebula with rotating bipolar jets. It has long been assumed that jets like these arose from an interacting binary system. Indeed, the data reveal that the central star in Fleming 1 has a companion in a very close orbit. [PUBLICATION ABSTRACT] Stars are generally spherical, yet their gaseous envelopes often appear nonspherical when ejected near the end of their lives. This quirk is most notable during the planetary nebula phase, when these envelopes become ionized. Interactions among stars in a binary system are suspected to cause the asymmetry. In particular, a precessing accretion disk around a companion is believed to launch point-symmetric jets, as seen in the prototype Fleming 1. Our finding of a post-common-envelope binary nucleus in Fleming 1 confirms that this scenario is highly favorable. Similar binary interactions are therefore likely to explain these kinds of outflows in a large variety of systems. [PUBLICATION ABSTRACT] Not Single After AllPlanetary nebulae form toward the end of the lives of sunlike stars. They appear after the star has shed its outer layers, and radiation from what is left of it ionizes the surrounding medium. Using the Very Large Telescope in Chile, Boffin et al. (p. 773) obtained spectra of the star at the center of Fleming 1, a point-symmetric planetary nebula with rotating bipolar jets. It has long been assumed that jets like these arose from an interacting binary system. Indeed, the data reveal that the central star in Fleming 1 has a companion in a very close orbit. Stars are generally spherical, yet their gaseous envelopes often appear nonspherical when ejected near the end of their lives. This quirk is most notable during the planetary nebula phase, when these envelopes become ionized. Interactions among stars in a binary system are suspected to cause the asymmetry. In particular, a precessing accretion disk around a companion is believed to launch point-symmetric jets, as seen in the prototype Fleming 1. Our finding of a post-common-envelope binary nucleus in Fleming 1 confirms that this scenario is highly favorable. Similar binary interactions are therefore likely to explain these kinds of outflows in a large variety of systems. Not Single After All Planetary nebulae form toward the end of the lives of sunlike stars. They appear after the star has shed its outer layers, and radiation from what is left of it ionizes the surrounding medium. Using the Very Large Telescope in Chile, Boffin et al. (p. 773 ) obtained spectra of the star at the center of Fleming 1, a point-symmetric planetary nebula with rotating bipolar jets. It has long been assumed that jets like these arose from an interacting binary system. Indeed, the data reveal that the central star in Fleming 1 has a companion in a very close orbit. Spectra of a planetary nebula’s central star reveal a companion star responsible for launching the system’s rotating jets. Stars are generally spherical, yet their gaseous envelopes often appear nonspherical when ejected near the end of their lives. This quirk is most notable during the planetary nebula phase, when these envelopes become ionized. Interactions among stars in a binary system are suspected to cause the asymmetry. In particular, a precessing accretion disk around a companion is believed to launch point-symmetric jets, as seen in the prototype Fleming 1. Our finding of a post–common-envelope binary nucleus in Fleming 1 confirms that this scenario is highly favorable. Similar binary interactions are therefore likely to explain these kinds of outflows in a large variety of systems. |
| Author | JONES, David DAY-JONES, Avril C KÖPPEN, Joachim MISZALSKI, Brent CORRADI, Romano L. M RAUCH, Thomas BOFFIN, Henri M. J NAPIWOTZKI, Ralf |
| Author_xml | – sequence: 1 givenname: Henri M. J surname: BOFFIN fullname: BOFFIN, Henri M. J organization: European Southern Observatory (ESO), Alonso de Cordova 3107, Vitacura, Casilla 19001, Santiago, Chile – sequence: 2 givenname: Brent surname: MISZALSKI fullname: MISZALSKI, Brent organization: South African Astronomical Observatory (SAAO), Post Office Box 9, Observatory 7935, South Africa – sequence: 3 givenname: Thomas surname: RAUCH fullname: RAUCH, Thomas organization: Institute for Astronomy and Astrophysics, Kepler Center for Astro and Particle Physics, Eberhard Karls University, Sand 1, 72076 Tübingen, Germany – sequence: 4 givenname: David surname: JONES fullname: JONES, David organization: European Southern Observatory (ESO), Alonso de Cordova 3107, Vitacura, Casilla 19001, Santiago, Chile – sequence: 5 givenname: Romano L. M surname: CORRADI fullname: CORRADI, Romano L. M organization: Instituto de Astrofisica de Canarias, E-38200 La Laguna, Tenerife, Spain – sequence: 6 givenname: Ralf surname: NAPIWOTZKI fullname: NAPIWOTZKI, Ralf organization: Physics, Astronomy and Mathematics, University of Hertfordshire, Hatfield AL10 9AB, United Kingdom – sequence: 7 givenname: Avril C surname: DAY-JONES fullname: DAY-JONES, Avril C organization: Universidad de Chile, Santiago, Casilla 36-D, Chile – sequence: 8 givenname: Joachim surname: KÖPPEN fullname: KÖPPEN, Joachim organization: Observatoire de Strasbourg, 11 rue de l'université, 67000 Strasbourg, France |
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| Keywords | Planetary nebulae Asymmetry Astrophysical jets Accretion disks Binary stars Gaseous shell |
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| Snippet | Stars are generally spherical, yet their gaseous envelopes often appear nonspherical when ejected near the end of their lives. This quirk is most notable... Not Single After All Planetary nebulae form toward the end of the lives of sunlike stars. They appear after the star has shed its outer layers, and radiation... Planetary nebulae form toward the end of the lives of sunlike stars. They appear after the star has shed its outer layers, and radiation from what is left of... Not Single After AllPlanetary nebulae form toward the end of the lives of sunlike stars. They appear after the star has shed its outer layers, and radiation... |
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| SubjectTerms | Astronomy Astrophysics Binary system Binary systems Companion stars Earth, ocean, space Exact sciences and technology Faint blue stars (including blue stragglers), white dwarfs, degenerate stars, nuclei of planetary nebulae Interstellar medium (ism) and nebulae in milky way Jets Nebulae Normal stars (by class): general or individual Planetary nebulae Spectra Stars Stars & galaxies Stellar system evolution Stellar systems. Galactic and extragalactic objects and systems. The universe |
| Title | An Interacting Binary System Powers Precessing Outflows of an Evolved Star |
| URI | https://www.ncbi.nlm.nih.gov/pubmed/23139326 https://www.proquest.com/docview/1143954804 https://search.proquest.com/docview/1151037493 https://search.proquest.com/docview/1554950008 https://search.proquest.com/docview/1808127366 |
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