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http://inaoe.repositorioinstitucional.mx/jspui/handle/1009/1033| Probing atlas model atmospheres at high spectral resolution. Stellar synthesis and reference template validation | |
| EMANUELE BERTONE TARICCO MIGUEL Y ROSA MARIA CHAVEZ DAGOSTINO LINO HECTOR RODRIGUEZ MERINO | |
| Acceso Abierto | |
| Atribución-NoComercial-SinDerivadas | |
| Aims. The fast improvement of spectroscopic observations makes mandatory a strong effort on the theoretical side to better reproduce the spectral energy distribution (SED) of stars at high spectral resolution. In this regard, relying on the Kurucz Atlas/Synthe original codes we computed the Bluered library, consisting of 832 synthetic SED of stars, that cover a large parameter space at very high spectral resolution (R = 500 000) along the 3500−7000 Å wavelength range. Methods. Bluered synthetic spectra have been used to assess in finer detail the intrinsic reliability and the performance limits of the Atlas theoretical framework. The continuum-normalized spectra of the Sun, Arcturus, and Vega, plus a selected list of 45 bright stars with high-quality SEDs from the Prugniel & Soubiran Elodie catalog, form our sample designed to probe the global properties of synthetic spectra across the entire range of H-R parameters. Results. Atlas models display a better fitting performance with increasing stellar temperature. High-resolution spectra of Vega, the Sun, and Arcturus have been reproduced at R = 100 000, respectively, within a 0.7%, 4.5%, and 8.8% relative scatter in residual flux. In all the three cases, the residual flux distribution shows a significant asymmetry (skewness parameter γ = −2.21, −0.98, −0.67, respectively), which neatly confirms an overall “excess” of theoretical line blanketing. For the Sun, this apparent discrepancy is alleviated, but not recovered, by a systematic decrease (−40%) of the line oscillator strengths, log(ɡf ), especially referring to iron transitions. Definitely, a straight “astrophysical” determination of log(ɡf) for each individual atomic transition has to be devised to overcome the problem. By neglecting overblanketing effects in theoretical models when fitting high-resolution continuum-normalized spectra of real stars, we lead to a systematically warmer effective temperature (between +80 and +300 K for the solar fit) and a slightly poorer metal content. | |
| Astronomy and Astrophysics | |
| 2008 | |
| Artículo | |
| Inglés | |
| Estudiantes Investigadores Público en general | |
| Bertone, E., et al., (2008). Probing atlas model atmospheres at high spectral resolution stellar synthesis and reference template validation, Astronomy and Astrophysics, Vol.485(3):823-835 | |
| ASTRONOMÍA Y ASTROFÍSICA | |
| Versión aceptada | |
| acceptedVersion - Versión aceptada | |
| Aparece en las colecciones: | Artículos de Astrofísica |
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| 10_Probing ATLAS model atmospheres.pdf | 3.09 MB | Adobe PDF | Visualizar/Abrir |