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نویسندگان مقالات پربازدید :
اخترفیزیک و علوم فضایی 2013
جزئیات رویداد
اینستاگرام تی پی بین
همایش ، رویداد ، ژورنال
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  • discovery of a coherent oscillation with a 1.07 h period in the suspected cataclysmic variable fbs 1220+753 (dra 7)

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    • تاریخ ارائه: 1392/07/24
    • تاریخ انتشار در تی پی بین: 1392/07/24
    • تعداد بازدید: 931
    • تعداد پرسش و پاسخ ها: 0
    • شماره تماس دبیرخانه رویداد: -
     we report results of extensive photometry of the suspected cataclysmic variable fbs 1220+753. the observations were obtained over 28 nights in 2010, 2011 and 2012. the total duration of the observations was 160 h. we clearly detected the highly coherent oscillation with a period of 1.0712887±0.0000013 h and a stable semi-amplitude of 0.03 mag. in a time scale of years, the oscillation period is very stable (dp/dt<(4.1±1.4)×10−10). the light curves of fbs 1220+753 show no obvious flickering. the significant brightness changes on large time intervals are also absent. therefore, it is unlikely that fbs 1220+753 is a cataclysmic variable. the period is compatible with oscillations seen in δ sct variables. but its high stability and the unchangeable oscillation amplitude suggest that the oscillation cannot be caused by multiperiodic stellar pulsations. the average pulse shape of the oscillation is very sinusoidal with slightly sharper maxima compared with minima, but it is somewhat changeable from year to year. the light curves obtained in 2011 and folded with the doubled oscillation period reveal that the adjacent oscillation cycles have slightly different depths of the minima and different steepness of the rise and decline. this behaviour resembles the behaviour of the binary subdwarf–white dwarf systems, in which the variability is caused by ellipsoidal variations. however, the folded light curve obtained from the data of 2010 reveal nearly equal shapes of the adjacent oscillation cycles, and this does not conform to such an interpretation. thus, the nature of the oscillation seen in fbs 1220+753 remains puzzling. to solve this puzzle, detailed spectroscopic observations are needed.

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