Comparative modelling of the spectra of cool giants
<i>Context.<i/> Our ability to extract information from the spectra of stars depends on reliable models of stellar atmospheres and appropriate techniques for spectral synthesis. Various model codes and strategies for the analysis of stellar spectra are available today.<i>Aims.<i...
Gespeichert in:
| Hauptverfasser: | , |
|---|---|
| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
06 November 2012
|
| In: |
Astronomy and astrophysics
Year: 2012, Jahrgang: 547 |
| ISSN: | 1432-0746 |
| DOI: | 10.1051/0004-6361/201219142 |
| Online-Zugang: | Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1051/0004-6361/201219142 Verlag, kostenfrei, Volltext: https://www.aanda.org/articles/aa/abs/2012/11/aa19142-12/aa19142-12.html 
|
| Verfasserangaben: | T. Lebzelter, U. Heiter, C. Abia, K. Eriksson, M. Ireland, H. Neilson, W. Nowotny, J. Maldonado, T. Merle, R. Peterson, B. Plez, C. I. Short, G. M. Wahlgren, C. Worley, B. Aringer, S. Bladh, P. de Laverny, A. Goswami, A. Mora, R. P. Norris, A. Recio-Blanco, M. Scholz, F. Thévenin, T. Tsuji, G. Kordopatis, B. Montesinos, and R. F. Wing |
MARC
| LEADER | 00000caa a2200000 c 4500 | ||
|---|---|---|---|
| 001 | 1571973230 | ||
| 003 | DE-627 | ||
| 005 | 20220814112956.0 | ||
| 007 | cr uuu---uuuuu | ||
| 008 | 180412s2012 xx |||||o 00| ||eng c | ||
| 024 | 7 | |a 10.1051/0004-6361/201219142 |2 doi | |
| 035 | |a (DE-627)1571973230 | ||
| 035 | |a (DE-576)501973230 | ||
| 035 | |a (DE-599)BSZ501973230 | ||
| 035 | |a (OCoLC)1341003808 | ||
| 040 | |a DE-627 |b ger |c DE-627 |e rda | ||
| 041 | |a eng | ||
| 084 | |a 29 |2 sdnb | ||
| 100 | 1 | |a Lebzelter, Thomas |d 1970- |e VerfasserIn |0 (DE-588)1155980158 |0 (DE-627)1018527605 |0 (DE-576)501972390 |4 aut | |
| 245 | 1 | 0 | |a Comparative modelling of the spectra of cool giants |c T. Lebzelter, U. Heiter, C. Abia, K. Eriksson, M. Ireland, H. Neilson, W. Nowotny, J. Maldonado, T. Merle, R. Peterson, B. Plez, C. I. Short, G. M. Wahlgren, C. Worley, B. Aringer, S. Bladh, P. de Laverny, A. Goswami, A. Mora, R. P. Norris, A. Recio-Blanco, M. Scholz, F. Thévenin, T. Tsuji, G. Kordopatis, B. Montesinos, and R. F. Wing |
| 264 | 1 | |c 06 November 2012 | |
| 300 | |a 30 | ||
| 336 | |a Text |b txt |2 rdacontent | ||
| 337 | |a Computermedien |b c |2 rdamedia | ||
| 338 | |a Online-Ressource |b cr |2 rdacarrier | ||
| 500 | |a Gesehen am 12.04.2018 | ||
| 520 | |a <i>Context.<i/> Our ability to extract information from the spectra of stars depends on reliable models of stellar atmospheres and appropriate techniques for spectral synthesis. Various model codes and strategies for the analysis of stellar spectra are available today.<i>Aims.<i/> We aim to compare the results of deriving stellar parameters using different atmosphere models and different analysis strategies. The focus is set on high-resolution spectroscopy of cool giant stars.<i>Methods.<i/> Spectra representing four cool giant stars were made available to various groups and individuals working in the area of spectral synthesis, asking them to derive stellar parameters from the data provided. The results were discussed at a workshop in Vienna in 2010. Most of the major codes currently used in the astronomical community for analyses of stellar spectra were included in this experiment.<i>Results.<i/> We present the results from the different groups, as well as an additional experiment comparing the synthetic spectra produced by various codes for a given set of stellar parameters. Similarities and differences of the results are discussed. <i>Conclusions.<i/> Several valid approaches to analyze a given spectrum of a star result in quite a wide range of solutions. The main causes for the differences in parameters derived by different groups seem to lie in the physical input data and in the details of the analysis method. This clearly shows how far from a definitive abundance analysis we still are. | ||
| 700 | 1 | |a Scholz, Michael |e VerfasserIn |0 (DE-588)1018079041 |0 (DE-627)690509111 |0 (DE-576)354957287 |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |t Astronomy and astrophysics |d Les Ulis : EDP Sciences, 1969 |g 547(2012) Artikel-Nummer A108, 30 Seiten |h Online-Ressource |w (DE-627)253390222 |w (DE-600)1458466-9 |w (DE-576)072283351 |x 1432-0746 |7 nnas |a Comparative modelling of the spectra of cool giants |
| 773 | 1 | 8 | |g volume:547 |g year:2012 |g extent:30 |a Comparative modelling of the spectra of cool giants |
| 856 | 4 | 0 | |u http://dx.doi.org/10.1051/0004-6361/201219142 |x Verlag |x Resolving-System |z kostenfrei |3 Volltext |
| 856 | 4 | 0 | |u https://www.aanda.org/articles/aa/abs/2012/11/aa19142-12/aa19142-12.html |x Verlag |z kostenfrei |3 Volltext |
| 951 | |a AR | ||
| 992 | |a 20180412 | ||
| 993 | |a Article | ||
| 994 | |a 2012 | ||
| 998 | |g 1018079041 |a Scholz, Michael |m 1018079041:Scholz, Michael |d 700000 |d 714000 |e 700000PS1018079041 |e 714000PS1018079041 |k 0/700000/ |k 1/700000/714000/ |p 22 | ||
| 999 | |a KXP-PPN1571973230 |e 3005977536 | ||
| BIB | |a Y | ||
| SER | |a journal | ||
| JSO | |a {"type":{"media":"Online-Ressource","bibl":"article-journal"},"note":["Gesehen am 12.04.2018"],"recId":"1571973230","language":["eng"],"person":[{"role":"aut","roleDisplay":"VerfasserIn","display":"Lebzelter, Thomas","given":"Thomas","family":"Lebzelter"},{"given":"Michael","family":"Scholz","role":"aut","roleDisplay":"VerfasserIn","display":"Scholz, Michael"}],"title":[{"title_sort":"Comparative modelling of the spectra of cool giants","title":"Comparative modelling of the spectra of cool giants"}],"physDesc":[{"extent":"30 S."}],"relHost":[{"physDesc":[{"extent":"Online-Ressource"}],"id":{"zdb":["1458466-9"],"eki":["253390222"],"issn":["1432-0746"]},"origin":[{"publisherPlace":"Les Ulis ; Berlin ; Heidelberg","dateIssuedDisp":"1969-","dateIssuedKey":"1969","publisher":"EDP Sciences ; Springer"}],"name":{"displayForm":["European Southern Observatory (ESO)"]},"part":{"text":"547(2012) Artikel-Nummer A108, 30 Seiten","volume":"547","extent":"30","year":"2012"},"titleAlt":[{"title":"Astronomy & astrophysics"},{"title":"a European journal"}],"pubHistory":["1.1969 -"],"corporate":[{"role":"isb","display":"European Southern Observatory","roleDisplay":"Herausgebendes Organ"}],"language":["eng"],"recId":"253390222","disp":"Comparative modelling of the spectra of cool giantsAstronomy and astrophysics","note":["Gesehen am 21.06.2024","Erscheint 36mal jährlich in 12 Bänden zu je 3 Ausgaben","Fortsetzung der Druck-Ausgabe"],"type":{"bibl":"periodical","media":"Online-Ressource"},"title":[{"subtitle":"an international weekly journal","title":"Astronomy and astrophysics","title_sort":"Astronomy and astrophysics"}]}],"name":{"displayForm":["T. Lebzelter, U. Heiter, C. Abia, K. Eriksson, M. Ireland, H. Neilson, W. Nowotny, J. Maldonado, T. Merle, R. Peterson, B. Plez, C. I. Short, G. M. Wahlgren, C. Worley, B. Aringer, S. Bladh, P. de Laverny, A. Goswami, A. Mora, R. P. Norris, A. Recio-Blanco, M. Scholz, F. Thévenin, T. Tsuji, G. Kordopatis, B. Montesinos, and R. F. Wing"]},"origin":[{"dateIssuedDisp":"06 November 2012","dateIssuedKey":"2012"}],"id":{"eki":["1571973230"],"doi":["10.1051/0004-6361/201219142"]}} | ||
| SRT | |a LEBZELTERTCOMPARATIV0620 | ||