THE ABSOLUTE PARAMETERS FOR NSVS 11868841 AND THE OVERSIZED STARS IN LOW-MASS ECLIPSING BINARIES
Fuente:
Redalyc
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Artículo científico |
| Sprache: | en |
| Veröffentlicht: |
Universidad Nacional Autónoma de México
2010
|
| Schlagworte: | |
| Online-Zugang: | |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| _version_ | 1876432082672025600 |
|---|---|
| author | Ö. Çakirli |
| author_facet | Ö. Çakirli |
| contents | THE ABSOLUTE PARAMETERS FOR NSVS 11868841 AND THE OVERSIZED STARS IN LOW-MASS ECLIPSING BINARIES Ö. Çakirli C. Ibanoglu A. Dervisoglu Física, Astronomía y Matemáticas mass stars: low stars: activity Binaries: eclipsing stars: fundamental parameters Spectroscopic observations of the low-mass eclipsing binary NSVS 11868841 have been obtained and the radial velocities were derived for both components. The masses and radii determined for the components are M1 = 0.870 ± 0.074 M¿, M2 = 0.607±0.053 M¿ and R1 = 0.983±0.030 R¿, R2 = 0.901±0.026 R¿. Both the primary and secondary stars' radii are 10% and 57% larger than those of zeroage- main-sequence stars with the same masses. This discrepancy may arise from the large spot coverage of both stars. We collected absolute parameters of 21 low mass double-lined eclipsing binaries and compared their positions in the mass-radius and mass-effective temperature panels. The large radii and lower effective temperatures found for NSV 11868841 are solved neither with differences in metallicity nor in mixing length parameters. These discrepancies for low mass stars may be due to magnetic fields inhibiting the convective energy transport, which lead to a large magnetic spot coverage of the surface of such low mass stars. 2010 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57115522015 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Num.2 Vol.46 |
| format | Artículo científico |
| id | redalyc_57115522015 |
| institution | Redalyc |
| language | en |
| publishDate | 2010 |
| publisher | Universidad Nacional Autónoma de México |
| spellingShingle | THE ABSOLUTE PARAMETERS FOR NSVS 11868841 AND THE OVERSIZED STARS IN LOW-MASS ECLIPSING BINARIES Ö. Çakirli Física, Astronomía y Matemáticas mass stars: low stars: activity Binaries: eclipsing stars: fundamental parameters THE ABSOLUTE PARAMETERS FOR NSVS 11868841 AND THE OVERSIZED STARS IN LOW-MASS ECLIPSING BINARIES Ö. Çakirli C. Ibanoglu A. Dervisoglu Física, Astronomía y Matemáticas mass stars: low stars: activity Binaries: eclipsing stars: fundamental parameters Spectroscopic observations of the low-mass eclipsing binary NSVS 11868841 have been obtained and the radial velocities were derived for both components. The masses and radii determined for the components are M1 = 0.870 ± 0.074 M¿, M2 = 0.607±0.053 M¿ and R1 = 0.983±0.030 R¿, R2 = 0.901±0.026 R¿. Both the primary and secondary stars' radii are 10% and 57% larger than those of zeroage- main-sequence stars with the same masses. This discrepancy may arise from the large spot coverage of both stars. We collected absolute parameters of 21 low mass double-lined eclipsing binaries and compared their positions in the mass-radius and mass-effective temperature panels. The large radii and lower effective temperatures found for NSV 11868841 are solved neither with differences in metallicity nor in mixing length parameters. These discrepancies for low mass stars may be due to magnetic fields inhibiting the convective energy transport, which lead to a large magnetic spot coverage of the surface of such low mass stars. 2010 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57115522015 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Num.2 Vol.46 |
| title | THE ABSOLUTE PARAMETERS FOR NSVS 11868841 AND THE OVERSIZED STARS IN LOW-MASS ECLIPSING BINARIES |
| topic | Física, Astronomía y Matemáticas mass stars: low stars: activity Binaries: eclipsing stars: fundamental parameters |
| url | https://www.redalyc.org/articulo.oa?id=57115522015 |