Pregled bibliografske jedinice broj: 176549
High-S/N, high-resolution spectroscopy of an eclipsed Beta Cephei star - HD 92024
High-S/N, high-resolution spectroscopy of an eclipsed Beta Cephei star - HD 92024 // The journal of astronomical data, 10 (2004), 2-20 (podatak o recenziji nije dostupan, članak, znanstveni)
CROSBI ID: 176549 Za ispravke kontaktirajte CROSBI podršku putem web obrasca
Naslov
High-S/N, high-resolution spectroscopy of an eclipsed Beta Cephei star - HD 92024
Autori
Hensberge, H. ; Sterken, C. ; Freyhammer, L.M. ; Pavlovski, Krešimir ; Ilijić, Saša ; Smette, A.
Izvornik
The journal of astronomical data (1385-3945) 10
(2004);
2-20
Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni
Ključne riječi
eclipsing binaries; variable stars; Beta Cep stars
(eclipsing binaries; variable stars; Beta Cep star)
Sažetak
We present spectroscopic data from a recent orbital analysis of the eclipsing SB-1 type binary system HD 92024 which has a Beta Cephei component. Fully reduced spectra are given together with technical details from the analysis, published elsewhere. In addition, a graphical representation of a high-S/N time-averaged spectrum is provided with line identifications. The spectra show profound variability caused by stellar pulsations, which is essential for application in asteroseismology but disturbing for the dynamical analysis. Orbital elements derived from the spectra with a procedure devised to minimise influence from these line-profile variations are found to be more precise than when using classical methods. A line-variability indicator is described and then used to guide a selection of spectral line-regions rich in information on the stellar Beta Cephei oscillations. Two lines are examined as examples.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
POVEZANOST RADA
Ustanove:
Fakultet elektrotehnike i računarstva, Zagreb,
Prirodoslovno-matematički fakultet, Zagreb