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相关论文: RR Lyrae Studies with Kepler

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We examined the complete short cadence sample of Kepler RR Lyrae stars to further investigate the recently discovered dynamical effects such as period doubling and additional modes. Here we present the findings on four stars. V450 Lyr may…

太阳与恒星天体物理 · 物理学 2015-06-17 L. Molnár , J. M. Benkő , R. Szabó , Z. Kolláth

We present new large samples of Galactic Cepheids and RR Lyrae stars from the OGLE Galaxy Variability Survey.

太阳与恒星天体物理 · 物理学 2017-09-13 Andrzej Udalski

The study of RR Lyrae stars has recently been invigorated thanks to the long, uninterrupted, ultra-precise time series data provided by the Kepler and CoRoT space telescopes. We give a brief overview of the new observational findings…

太阳与恒星天体物理 · 物理学 2015-10-21 R. Szabó , J. M. Benkő , M. Paparó , E. Chapellier , E. Poretti , A. Baglin , W. W. Weiss , K. Kolenberg , E. Guggenberger , J. -F. Le Borgne

We use asteroseismic data obtained by the NASA Kepler Mission to estimate the fundamental properties of more than 500 main-sequence and sub-giant stars. Data obtained during the first 10 months of Kepler science operations were used for…

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

The NASA Kepler and follow-on K2 missions (2009-2018) left a legacy of data and discoveries, finding thousands of exoplanets, and also obtaining high-precision long time-series data for hundreds of thousands of stars, including many types…

太阳与恒星天体物理 · 物理学 2021-08-29 Joyce Ann Guzik

Ranked near the top of the long list of exciting discoveries made with NASA's Kepler photometer is the detection of transiting circumbinary planets. In just over a year the number of such planets went from zero to seven, including a…

地球与行星天体物理 · 物理学 2015-06-17 William F. Welsh , Jerome A. Orosz , Joshua A. Carter , Daniel C. Fabrycky

The Kepler mission observed many thousands of red giants. The long time series, some as long as the mission itself, have allowed us to study red giants with unprecedented detail. Given that red giants are intrinsically luminous, and hence…

太阳与恒星天体物理 · 物理学 2020-06-29 Sarbani Basu , Saskia Hekker

Kepler Mission results are rapidly contributing to fundamentally new discoveries in both the exoplanet and asteroseismology fields. The data returned from Kepler are unique in terms of the number of stars observed, precision of photometry…

Asteroseismology allows us to probe the internal structure of stars through their global modes of oscillation. Thanks to missions such as the NASA Kepler space observatory, we now have high-quality asteroseismic data for nearly 100…

太阳与恒星天体物理 · 物理学 2020-01-15 Earl Patrick Bellinger

RR Lyrae stars being distance indicators and tracers of old population serve as excellent probes of the structure, formation, and evolution of our Galaxy. Thousands of them are being discovered in ongoing wide-field surveys. The OGLE…

星系天体物理 · 物理学 2016-09-07 Pawel Pietrukowicz , OGLE collaboration

Discovery of binary systems among RR Lyrae stars belongs to challenges of present astronomy. So far, none of classical RR Lyrae stars was clearly confirmed that it is a part of an eclipsing system. For this reason we studied two RR Lyrae…

太阳与恒星天体物理 · 物理学 2016-01-14 J. Liska , M. Skarka , P. Hajkova , R. F. Auer

Purpose: RR Lyrae stars are important distance indicators. They are usually present in globular clusters where they were first discovered. The study of their properties and distribution in our Galaxy and external galaxies constitutes a…

星系天体物理 · 物理学 2025-02-20 Roberto Capuzzo-Dolcetta

The successful launches of the CoRoT and Kepler space missions have led to the detections of solar-like oscillations in large samples of red-giant stars. The large numbers of red giants with observed oscillations make it possible to…

太阳与恒星天体物理 · 物理学 2011-09-02 S. Hekker , R. L. Gilliland , Sarbani Basu , J. De Ridder , W. J. Chaplin , Y. Elsworth

Over the past nine years, the Kepler and K2 Missions have carried out high precision photometric monitoring of more than half a million stars. Among these targets are 29 clusters and associations, with ages from 1 Myr to over 11 Gyr. We…

The popularity of pulsating stars resides in their capacity of determining several crucial and relevant parameters such as heliocentric distances, ages, metallicity gradients and reddening. RR Lyrae stars are old stellar tracers and have…

太阳与恒星天体物理 · 物理学 2024-09-10 Clara E. Martínez-Vázquez

Thousands of RR Lyrae stars have been observed by the \textit{Kepler} space telescope so far. We developed a photometric pipeline tailored to the light variations of these stars, called the Extended Aperture Photometry (EAP). We present the…

天体物理仪器与方法 · 物理学 2018-07-18 E. Plachy , L. Molnár , A. Bódi , M. Skarka , Á. L. Juhász , Á. Sódor , P. Klagyivik , R. Szabó

The NASA $Kepler$ mission obtained long-term high-quality photometric observations for a large number of stars in its original field of view from 2009 to 2013. In order to provide reliable stellar parameters in a homogeneous way, the LAMOST…

太阳与恒星天体物理 · 物理学 2020-11-11 J. N. Fu , P. De Cat , W. Zong , A. Frasca , R. O. Gray , A. B. Ren , J. Molenda-Żakowicz , C. J. Corbally , G. Catanzaro , J. R. Shi , A. L. Luo , H. T. Zhang

Aims: To try and clarify whether there are stars in the neighbourhood of $\beta$ Lyrae which are physically connected to the famous prototype eclipsing binary. Methods: Scrutinize the astrometric and photometric data (from Hipparcos and…

太阳与恒星天体物理 · 物理学 2019-10-09 U. Bastian

NASA's re-purposed Kepler mission -- dubbed K2 -- has brought new scientific opportunities that were not anticipated for the original Kepler mission. One science goal that makes optimal use of K2's capabilities, in particular its 360-degree…