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相关论文: New CCD Photometry Study of RV UMa

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We present in this paper the new study of variable star AM Cnc, a short period RRab star, in orther to determine, through the light curve and the physical parameters. The Star were observed for a total of 293 sessions shooting, and exhibits…

太阳与恒星天体物理 · 物理学 2015-10-13 D. Tasselli

RV UMa is one of the most extensively studied RR Lyrae stars showing Blazhko modulation. Its photometric observations cover more than 90 years. The published photoelectric observations of RV UMa obtained at the Konkoly Observatory (Kanyo,…

天体物理学 · 物理学 2007-08-15 Zs. Hurta

Extended BV(RI)c CCD observations of SS Cnc, a short period RRab star are presented. Nearly 1400 data points in each band have been obtained spanning over 79 days during the spring of 2005. The star exhibits light curve modulation, the so…

天体物理学 · 物理学 2008-11-26 J. Jurcsik , B. Szeidl , Á. Sódor , I. Dékány , Zs. Hurta , K. Posztobányi , K. Vida , M. Váradi , A. Szing

RV UMa is one of the RRab stars showing regular large amplitude light curve modulation. Extended photoelectric observations of RV UMa obtained at the Konkoly Observatory were published by Kanyo (1976). The analysis of the data was published…

天体物理学 · 物理学 2009-11-13 Zs. Hurta , J. Jurcsik , B. Szeidl , A. Sodor

This study investigates periodic modulation of the light curve of the RRc star TV Boo and its physical parameters based on photometric data. This phenomenon, known as Blazhko effect, is quite rare among RRc stars. Frequency analysis based…

太阳与恒星天体物理 · 物理学 2014-06-18 M. Skarka , M. Zejda

Extended CCD monitoring of RR Gem revealed that it is a Blazhko type RRab star with the shortest Blazhko period (7.23d) and smallest modulation amplitude (Delta Mmax<0.1 mag) currently known. The short period of the modulation cycle enabled…

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

DM Cyg, a fundamental mode RRab star was observed in the 2007 and 2008 seasons in the frame of the Konkoly Blazhko Survey. Very small amplitude light curve modulation was detected with 10.57 d modulation period. The maximum brightness and…

太阳与恒星天体物理 · 物理学 2015-05-13 J. Jurcsik , Zs. Hurta , A. Sodor , B. Szeidl , I. Nagy , K. Posztobanyi , M. Varadi , K. Vida , B. Belucz , I. Dekany , G. Hajdu , Zs. Kovari , E. Kun

We analyzed the incidence and properties of RR Lyrae stars that show evidence for amplitude and phase modulation (the so-called Blazhko Effect) in a sample of $\sim$3,000 stars with LINEAR and ZTF light curve data collected during the…

太阳与恒星天体物理 · 物理学 2025-04-09 Ema Donev , Željko Ivezić

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

A thorough analysis of multicolour CCD observations of two modulated RRab-type variables, XY And and UZ Vir is presented. These Blazhko stars show relatively simple light-curve modulation with the usual multiplet structures in their Fourier…

太阳与恒星天体物理 · 物理学 2015-06-05 Á. Sódor , G. Hajdu , J. Jurcsik , B. Szeidl , K. Posztobányi , Zs. Hurta , B. Belucz , E. Kun

Among the tens of thousands of known RR Lyrae stars there are only a handful that show indications of possible binarity. The question why this is the case is still unsolved, and has recently sparked several studies dedicated to the search…

太阳与恒星天体物理 · 物理学 2015-12-04 Elisabeth Guggenberger , Thomas G. Barnes , Katrien Kolenberg

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

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

We present the results of multi-longitude observations of KV Cancri, an RR Lyrae star showing an irregular Blazhko effect. With a pulsation period of 0.50208 day, the times of light curve maxima are delayed by 6 minutes per day. This daily…

太阳与恒星天体物理 · 物理学 2013-10-17 Pierre de Ponthiere , Michel Bonnardeau , Franz-Joseph Hambsch , Tom Krajci , Kenneth Menzies , Richard Sabo

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

Using an image subtraction method we have searched for variable stars in the globular cluster M14. We confirmed 62 previously known catalogued variables. In addition to the previoulsy known variables we have identified 71 new variables. We…

太阳与恒星天体物理 · 物理学 2012-05-15 Kyle E. Conroy , Andrew N. Darragh , Zheyu J. Liu , Brian W. Murphy

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 present the first simultaneous photometric and spectroscopic investigation of a large set of RR Lyrae variables in a globular cluster. The radial-velocity data presented comprise the largest sample of RVs of RR Lyrae stars ever obtained.…

The amplitude and phase modulation observed in a significant fraction of the RR Lyrae variables - the Blazhko effect - represents a long-standing enigma in stellar pulsation theory. No satisfactory explanation for the Blazhko effect has…

太阳与恒星天体物理 · 物理学 2011-07-05 R. Smolec , P. Moskalik , K. Kolenberg , S. Bryson , M. T. Cote , R. L. Morris
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