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相关论文: Blazhko modulation in the infrared

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We briefly discuss three cases of RR~Lyrae variable stars with Blazhko modulation from the OGLE Galactic bulge collection. In one of the discussed stars modulation with two periods is detected, in other star, we detect three Blazhko…

太阳与恒星天体物理 · 物理学 2016-01-12 Karolina Bakowska , Radoslaw Smolec

We present the first results of our analyses of selected RR Lyrae stars for which data have been obtained by the Kepler Mission. As expected, we find a significant fraction of the RRab stars to show the Blazhko effect, a still unexplained…

We developed an Inverse Photometric method (IPM) to determine global physical parameters of RR Lyrae stars exclusively from multicolor light curves (S\'odor, Jurcsik & Szeidl, 2009, MNRAS, 394, 261). We showed that for good quality…

太阳与恒星天体物理 · 物理学 2010-04-13 Á. Sódor

Recent photometric space missions, such as CoRoT and Kepler revealed that many RR Lyrae stars pulsate -- beyond their main radial pulsation mode -- in low amplitude modes. Space data seem to indicate a clear trend, namely overtone (RRc)…

太阳与恒星天体物理 · 物理学 2015-08-19 J. M. Benkő , R. Szabó

Period study of 321 fundamental mode galactic field RR Lyrae type stars (RRab), which had appropriate data in ASAS and SuperWASP surveys, brighter than 12.5 mag in maximum light was performed. We found 100 stars to be definitely modulated.…

太阳与恒星天体物理 · 物理学 2015-06-18 Marek Skarka

A systematic survey to establish the true incidence rate of the Blazhko modulation among short-period, fundamental-mode, Galactic field RR Lyrae stars has been accomplished. The Konkoly Blazhko Survey (KBS) was initiated in 2004. Since then…

太阳与恒星天体物理 · 物理学 2015-05-13 J. Jurcsik , Á. Sódor , B. Szeidl , Zs. Hurta , M. Váradi , K. Posztobányi , K. Vida , G. Hajdu , Zs. Kővári , I. Nagy , L. Molnár , B. Belucz

Rapid and strong changes in the Blazhko modulation of RR Lyrae stars, as they have recently been detected in high precision satellite data, have become a crucial topic in finding an explanation of the long-standing mystery of the Blazhko…

We have performed a detailed study of the pulsational and evolutionary characteristics of 133 RR Lyrae stars in the globular cluster NGC5272 (M3) using highly accurate BVI data taken on 5 separate epochs. M3 seems to contain no less than…

天体物理学 · 物理学 2009-11-10 C. Cacciari , T. M. Corwin , B. W. Carney

In an extended photometric campaign of RR Lyrae variables of the globular cluster M3, an aberrant light-curve, non-Blazhko RRab star, V123, was detected. Based on its brightness, colors and radial velocity curve, V123 is a bona fide member…

太阳与恒星天体物理 · 物理学 2015-06-17 J. Jurcsik , P. Smitola , G. Hajdu , C. Pilachowski , K. Kolenberg , Á. Sódor , G. Fűrész , A. Moór , E. Kun , A. Saha , P. Prakash , P. Blum , I. Tóth

Thorough analysis of the multicolour CCD observations of the RRab-type variable, CZ Lacertae is presented. The observations were carried out in two consecutive observing seasons in 2004 and 2005 within the framework of the Konkoly Blazhko…

太阳与恒星天体物理 · 物理学 2015-05-20 Á. Sódor , J. Jurcsik , B. Szeidl , M. Váradi , A. Henden , K. Vida , Zs. Hurta , K. Posztobányi , I. Dékány , A. Szing

We found a possible relationship between the modulation period and the amplitude of the Blazhko RR Lyrae stars: long modulation period generally implies high modulation amplitude while the short modulation period results in small amplitude.…

太阳与恒星天体物理 · 物理学 2015-10-21 J. M. Benkő , R. Szabó

We present our results of searching for differences in light curves of modulated and non-modulated RRab stars in the Galactic bulge. We examined a sample of more than 8000 stars. The most important results are that Blazhko stars have…

太阳与恒星天体物理 · 物理学 2018-09-12 M. Skarka , Z. Prudil

In this paper it is shown that the Blazhko effect may result from a near-resonant type of multi-mode pulsation, where two (or sometimes more) periodic oscillations with slightly different frequencies gradually slip in phase, producing a…

太阳与恒星天体物理 · 物理学 2015-04-15 Paul H. Bryant

The period-change behaviour of 134 RR Lyrae stars in the globular cluster Messier 3 (M3) is investigated on the ~120-year time base of the photometric observations. The mean period-change rates (\beta \approx 0.01 d Myr^-1) of the…

太阳与恒星天体物理 · 物理学 2015-05-30 J. Jurcsik , G. Hajdu , B. Szeidl , K. Oláh , J. Kelemen , Á. Sódor , A. Saha , P. Mallick , J. Claver

The overtone and multi-mode RR Lyrae stars in the globular cluster M3 are studied using a 200-d long, $B,V$ and $I_{\mathrm C}$ time-series photometry obtained in 2012. 70\% of the 52 overtone variables observed show some kind of…

About a dozen field RR Lyrae stars have been observed with the 24-inch Heyde-Zeiss telescope of the Konkoly Observatory at Sv\'abhegy, Budapest, since its refurbishment in 2003. Most of the observing time is allocated for the investigation…

天体物理学 · 物理学 2009-11-13 Á. sódor

The analysis of recent, extended multicolour CCD and archive photoelectric, photographic and visual observations has revealed several important properties of RZ Lyr, an RRab-type variable exhibiting large-amplitude Blazhko modulation. On…

We search for signs of period doubling in CoRoT RR Lyrae stars. The occurrence of this dynamical effect in modulated RR Lyrae stars might help us to gain more information about the mysterious Blazhko effect. The temporal variability of the…

太阳与恒星天体物理 · 物理学 2014-11-05 R. Szabó , J. M. Benkő , M. Paparó , E. Chapellier , E. Poretti , A. Baglin , W. W. Weiss , K. Kolenberg , E. Guggenberger , J. -F. Le Borgne

The unprecedented photometric precision along with the quasi-continuous sampling provided by the Kepler space telescope revealed new and unpredicted phenomena that reformed and invigorated RR Lyrae star research. The discovery of period…

太阳与恒星天体物理 · 物理学 2020-11-25 Emese Plachy , Róbert Szabó

The light curves of 50 RRab (RR0) stars in M5 collected in Paper I are investigated to detect Blazhko modulation. 18 Blazhko stars are identified, and modulation is suspected in two additional cases. The mean pulsation period of Blazhko…

太阳与恒星天体物理 · 物理学 2015-05-20 J. Jurcsik , B. Szeidl , C. Clement , Zs. Hurta , M. Lovas