Atmosphere tomography of red supergiant stars
3-D simulations suggest that the atmospheres of red supergiants are subject to large-amplitude convective motions, which are suspected to generate supersonic motions and shocks. We perform tomography of supergiant-star atmospheres, on temporal series of high-resolution spectra and on 3-D hydrodynami...
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Published in | EAS publications series Vol. 60; pp. 85 - 92 |
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Main Authors | , , , , |
Format | Journal Article |
Language | English |
Published |
Les Ulis
EDP Sciences
2013
|
Online Access | Get full text |
ISBN | 2759809978 9782759809974 |
ISSN | 1633-4760 1638-1963 |
DOI | 10.1051/eas/1360009 |
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Abstract | 3-D simulations suggest that the atmospheres of red supergiants are subject to large-amplitude convective motions, which are suspected to generate supersonic motions and shocks. We perform tomography of supergiant-star atmospheres, on temporal series of high-resolution spectra and on 3-D hydrodynamical synthetic spectra. The tomographic technique is improved by the computation of the contribution function, which is used to construct numerical spectral masks probing different optical depths. This exploratory work allows us to put spatial and temporal constraints on velocity fields predicted by 3-D model atmospheres. |
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AbstractList | 3-D simulations suggest that the atmospheres of red supergiants are subject to large-amplitude convective motions, which are suspected to generate supersonic motions and shocks. We perform tomography of supergiant-star atmospheres, on temporal series of high-resolution spectra and on 3-D hydrodynamical synthetic spectra. The tomographic technique is improved by the computation of the contribution function, which is used to construct numerical spectral masks probing different optical depths. This exploratory work allows us to put spatial and temporal constraints on velocity fields predicted by 3-D model atmospheres. 3-D simulations suggest that the atmospheres of red supergiants are subject to large-amplitude convective motions, which are suspected to generate supersonic motions and shocks. We perform tomography of supergiant-star atmospheres, on temporal series of high-resolution spectra and on 3-D hydrodynamical synthetic spectra. The tomographic technique is improved by the computation of the contribution function, which is used to construct numerical spectral masks probing different optical depths. This exploratory work allows us to put spatial and temporal constraints on velocity fields predicted by 3-D model atmospheres. [PUBLICATION ABSTRACT] |
Author | Chiavassa, A. Van Eck, S. Plez, B. Lion, S. Jorissen, A. |
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Cites_doi | 10.1002/1521-3994(200208)323:3/4<213::AID-ASNA213>3.0.CO;2-H 10.1051/0004-6361:20078096 10.1051/0004-6361:20011294 10.1051/0004-6361/200911780 10.1051/0004-6361:20011261 10.1051/0004-6361:20066353 10.1016/j.jcp.2011.09.026 10.1088/0004-6256/135/4/1450 10.1051/0004-6361:200809724 10.1007/978-1-4757-3876-6 10.1051/0004-6361/201015435 10.1111/j.1365-2966.2006.10973.x 10.1086/430901 10.1051/0004-6361/201015768 10.1051/0004-6361/201117463 |
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Editor | Kervella, P. Le Bertre, T. Perrin, G. |
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References | Chiavassa (R7) 2011; 528 Alvarez (R3) 2000; 362 Raskin (R19) 2011; 526 Gustafsson (R13) 2008; 486 Freytag (R11) 2012; 231 Magain (R18) 1986; 163 Freytag (R9) 2002; 323 Alvarez (R5) 2001; 379 R14 Josselin (R15) 2007; 469 Levesque (R17) 2005; 628 Chiavassa (R6) 2009; 506 Freytag (R10) 2008; 483 Albrow (R1) 1996; 278 Alvarez (R2) 1998; 330 Chiavassa (R8) 2011; 535 Alvarez (R4) 2001; 379 Kiss (R16) 2006; 372 Gray (R12) 2008; 135 |
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