1,223 research outputs found

    Discovery of Delta Scuti variables in eclipsing binary systems II.Southern TESS field search

    Full text link
    The presence of pulsating stars in eclipsing binary systems (EBs) makes these objects significant since they allow us to investigate the stellar interior structure and evolution. Different types of pulsating stars could be found in EBs such as Delta Scuti variables. Delta Scuti stars in EBs have been known for decades and the increasing number of such systems is important for understanding pulsational structure. Hence, in this study, a research was carried out on the southern TESS field to discover new Delta Scuti stars in EBs. We produced an algorithm to search for detached and semi-detached EBs considering three steps; the orbital period (Porb_{orb})'s harmonics in the Fourier spectrum, skewness of the light curves, and classification of \textsc{UPSILON} program. If two of these steps classify a system as an EB, the algorithm also identifies it as an EB. The TESS pixel files of targets were also analyzed to see whether the fluxes are contaminated by other systems. No contamination was found. We researched the existence of pulsation through EBs with a visual inspection. To confirm Delta Scuti-type oscillations, the binary variation was removed from the light curve, and residuals were analyzed. Consequently, we identified 42 Delta Scuti candidates in EBs. The Porb_{orb}, LL, and MV_{V} of systems were calculated. Their positions on the H-R diagram and the known orbital-pulsation period relationship were analyzed. We also examined our targets to find if any of them show frequency modulation with the orbital period and discovered one candidate of tidally tilted pulsators.Comment: Published in MNRA

    Agricultural Academy

    Get PDF
    Abstract DOGAN, I. S., O. YIlDIz, E. EYDurAN and S. KOSE, 2011. A study on determination of functional food consumption habits and awareness of consumers in Turkey. Bulg. J. Agric. Sci., The survey study was to determine the status of knowledge about functional foods, the factors influencing consumer preferences in the purchase and their expectations in Turkey. A total of 389 persons, 288 men and 101 women ranging from 10 to 70 ages were participated in the study. Participants' level of awareness about functional foods was found to be approximately 40%. In general, it was determined that these foods were consumed little by almost half (51.34%) of those participated to the survey. It was also found that women and especially participants ranging from 20 to 40 years-old consumed more functional foods than the rest of participants. As a result, it was concluded that education, income level, product price, compliance with religious sensitivities, the presence of artificial food additives and genetic modification were to be effective on functional food choice

    MICROSTRUCTURAL STABILITY AND OXIDATION RESISTANCE OF 9-12 CHROMIUM STEELS AT ELEVATED TEMPERATURES

    Get PDF
    ABSTRACT Various martensitic 9-12 Cr steels are utilized currently in fossil fuel powered energy plants for their good elevated temperature properties such as creep strength, steam side oxidation resistance, fire side corrosion resistance, and thermal fatigue resistance. Need for further improvements on the properties of 9-12 Cr steels for higher temperature (>600 o C) use is driven by the environmental concerns (i.e., improve efficiency to reduce emissions and fossil fuel consumption). In this paper, we will discuss the results of the research done to explore new subsitutional solute solution and precipitate hardening mechanisms for improved strength of 9-12 Cr martensitic steels. Stability of the phases present in the steels will be evaluated for various temperature and time exposures. A comparison of microstructural properties of the experimental steels and commercial steels will also be presented

    Characterizing two solar-type Kepler subgiants with asteroseismology: KIC10920273 and KIC11395018

    Full text link
    Determining fundamental properties of stars through stellar modeling has improved substantially due to recent advances in asteroseismology. Thanks to the unprecedented data quality obtained by space missions, particularly CoRoT and Kepler, invaluable information is extracted from the high-precision stellar oscillation frequencies, which provide very strong constraints on possible stellar models for a given set of classical observations. In this work, we have characterized two relatively faint stars, KIC10920273 and KIC11395018, using oscillation data from Kepler photometry and atmospheric constraints from ground-based spectroscopy. Both stars have very similar atmospheric properties; however, using the individual frequencies extracted from the Kepler data, we have determined quite distinct global properties, with increased precision compared to that of earlier results. We found that both stars have left the main sequence and characterized them as follows: KIC10920273 is a one-solar-mass star (M=1.00 +/- 0.04 M_sun), but much older than our Sun (t=7.12 +/- 0.47 Gyr), while KIC11395018 is significantly more massive than the Sun (M=1.27 +/- 0.04 M_sun) with an age close to that of the Sun (t=4.57 +/- 0.23 Gyr). We confirm that the high lithium abundance reported for these stars should not be considered to represent young ages, as we precisely determined them to be evolved subgiants. We discuss the use of surface lithium abundance, rotation and activity relations as potential age diagnostics.Comment: 12 pages, 3 figures, 5 tables. Accepted by Ap
    • …
    corecore