Light Curve Modeling of Eclipsing Binary Stars:
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
New York, NY
Springer New York
1993
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| Schlagworte: | |
| Online-Zugang: | Volltext |
| Beschreibung: | In the two decades since the development of the first eclipsing-binary modeling code, new analytic techniques and the availability of powerful, sometimes dedicated computing facilities have made possible vastly improved determinations of fundamental and even transient stellar parameters. The scale of these developments, of course, raises questions about modeling tools, techniques, and philosophies, such as: Who will maintain and upgrade the codes? Will the codes be open to improvement by outsiders, and if so, how? And, indeed, what should be the goals of a modeling program? Such questions had not been aired for a long time and, for this reason alone, deserved to be discussed in as general a forum as the community provides. This volume contains material presented by Commission 42 (Close Binary Stars) during the International Astronomical Union's XXI General Assembly in Argentina, July 1991, and during IAU Colloquium 151, Cordoba, Argentina, August 1991. The techniques discussed include simulations of stellar bright and dark spots, streams, partial and complete stellar disks, prominences, and other features characterizing active stars; modeling of polarization parameters; models that use radial velocities as well as line profile simulations to model velocity field variation across stellar disks; the weighted effects of brightness asymmetries; and models for translucent eclipsing agents such as stellar winds |
| Beschreibung: | 1 Online-Ressource (VI, 202p. 43 illus) |
| ISBN: | 9781461227427 9781461276494 |
| DOI: | 10.1007/978-1-4612-2742-7 |
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| 500 | |a In the two decades since the development of the first eclipsing-binary modeling code, new analytic techniques and the availability of powerful, sometimes dedicated computing facilities have made possible vastly improved determinations of fundamental and even transient stellar parameters. The scale of these developments, of course, raises questions about modeling tools, techniques, and philosophies, such as: Who will maintain and upgrade the codes? Will the codes be open to improvement by outsiders, and if so, how? And, indeed, what should be the goals of a modeling program? Such questions had not been aired for a long time and, for this reason alone, deserved to be discussed in as general a forum as the community provides. This volume contains material presented by Commission 42 (Close Binary Stars) during the International Astronomical Union's XXI General Assembly in Argentina, July 1991, and during IAU Colloquium 151, Cordoba, Argentina, August 1991. The techniques discussed include simulations of stellar bright and dark spots, streams, partial and complete stellar disks, prominences, and other features characterizing active stars; modeling of polarization parameters; models that use radial velocities as well as line profile simulations to model velocity field variation across stellar disks; the weighted effects of brightness asymmetries; and models for translucent eclipsing agents such as stellar winds | ||
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| spelling | Milone, E. F. Verfasser aut Light Curve Modeling of Eclipsing Binary Stars edited by E. F. Milone New York, NY Springer New York 1993 1 Online-Ressource (VI, 202p. 43 illus) txt rdacontent c rdamedia cr rdacarrier In the two decades since the development of the first eclipsing-binary modeling code, new analytic techniques and the availability of powerful, sometimes dedicated computing facilities have made possible vastly improved determinations of fundamental and even transient stellar parameters. The scale of these developments, of course, raises questions about modeling tools, techniques, and philosophies, such as: Who will maintain and upgrade the codes? Will the codes be open to improvement by outsiders, and if so, how? And, indeed, what should be the goals of a modeling program? Such questions had not been aired for a long time and, for this reason alone, deserved to be discussed in as general a forum as the community provides. This volume contains material presented by Commission 42 (Close Binary Stars) during the International Astronomical Union's XXI General Assembly in Argentina, July 1991, and during IAU Colloquium 151, Cordoba, Argentina, August 1991. The techniques discussed include simulations of stellar bright and dark spots, streams, partial and complete stellar disks, prominences, and other features characterizing active stars; modeling of polarization parameters; models that use radial velocities as well as line profile simulations to model velocity field variation across stellar disks; the weighted effects of brightness asymmetries; and models for translucent eclipsing agents such as stellar winds Physics Physical geography Astronomy, Observations and Techniques Astrophysics and Astroparticles Geophysics/Geodesy Lichtkurve (DE-588)4306547-8 gnd rswk-swf Bedeckungsveränderlicher (DE-588)4144255-6 gnd rswk-swf 1\p (DE-588)1071861417 Konferenzschrift 1991 Buenos Aires gnd-content Bedeckungsveränderlicher (DE-588)4144255-6 s Lichtkurve (DE-588)4306547-8 s 2\p DE-604 https://doi.org/10.1007/978-1-4612-2742-7 Verlag Volltext 1\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk 2\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk |
| spellingShingle | Milone, E. F. Light Curve Modeling of Eclipsing Binary Stars Physics Physical geography Astronomy, Observations and Techniques Astrophysics and Astroparticles Geophysics/Geodesy Lichtkurve (DE-588)4306547-8 gnd Bedeckungsveränderlicher (DE-588)4144255-6 gnd |
| subject_GND | (DE-588)4306547-8 (DE-588)4144255-6 (DE-588)1071861417 |
| title | Light Curve Modeling of Eclipsing Binary Stars |
| title_auth | Light Curve Modeling of Eclipsing Binary Stars |
| title_exact_search | Light Curve Modeling of Eclipsing Binary Stars |
| title_full | Light Curve Modeling of Eclipsing Binary Stars edited by E. F. Milone |
| title_fullStr | Light Curve Modeling of Eclipsing Binary Stars edited by E. F. Milone |
| title_full_unstemmed | Light Curve Modeling of Eclipsing Binary Stars edited by E. F. Milone |
| title_short | Light Curve Modeling of Eclipsing Binary Stars |
| title_sort | light curve modeling of eclipsing binary stars |
| topic | Physics Physical geography Astronomy, Observations and Techniques Astrophysics and Astroparticles Geophysics/Geodesy Lichtkurve (DE-588)4306547-8 gnd Bedeckungsveränderlicher (DE-588)4144255-6 gnd |
| topic_facet | Physics Physical geography Astronomy, Observations and Techniques Astrophysics and Astroparticles Geophysics/Geodesy Lichtkurve Bedeckungsveränderlicher Konferenzschrift 1991 Buenos Aires |
| url | https://doi.org/10.1007/978-1-4612-2742-7 |
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