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Context. Most stars from in groups which with time disperse, building the field population of their host galaxy. In the Milky Way, open clusters have been continuously forming in the disk up to the present time, providing it with stars…

Astrophysics of Galaxies · Physics 2023-09-08 Pedro Guilherme-Garcia , Alberto Krone-Martins , André Moitinho

The Kepler spacecraft is providing time series of photometric data with micromagnitude precision for hundreds of A-F type stars. We present a first general characterization of the pulsational behaviour of A-F type stars as observed in the…

About 22000 Kepler stars and nearly 60000 TESS stars from sectors 1-24 have been classified according to variability type. A large proportion of stars of all spectral types appear to have periods consistent with the expected rotation…

Solar and Stellar Astrophysics · Physics 2020-08-17 L. A. Balona

In order to understand stellar evolution, it is crucial to efficiently determine stellar surface rotation periods. An efficient tool to automatically determine reliable rotation periods is needed when dealing with large samples of stellar…

Solar and Stellar Astrophysics · Physics 2021-03-24 Sylvain N. Breton , Angela R. G. Santos , Lisa Bugnet , Savita Mathur , Rafael A. García , Pere L. Pallé

Studies of Galactic structure and evolution have benefitted enormously from Gaia kinematic information, though additional, intrinsic stellar parameters like age are required to best constrain Galactic models. Asteroseismology is the most…

As revealed by its peculiar Kepler light curve, the enigmatic star KIC 8462852 undergoes short and deep flux dimmings at a priori unrelated epochs. It presents nonetheless all other characteristics of a quiet 1 Gyr old F3V star. These…

Stellar surface rotation carries information about stellar parameters---particularly ages---and thus the large rotational datasets extracted from Kepler timeseries represent powerful probes of stellar populations. In this article, we…

Solar and Stellar Astrophysics · Physics 2019-02-27 Jennifer L. van Saders , Marc H. Pinsonneault , Mauro Barbieri

Dippers are typically low-mass, pre-main-sequence stars that display dips in their light curves. These dips have been attributed to dusty warps that form in the inner part of the disk. Our goal is to derive the properties of dipper stars in…

Solar and Stellar Astrophysics · Physics 2021-07-14 Noemi Roggero , Jérôme Bouvier , Luisa M. Rebull , Ann Marie Cody

We report rotation periods, variability characteristics, gyrochronological ages for ~950 of the Kepler Object of Interest host stars. We find a wide dispersion in the amplitude of the photometric variability as a function of rotation,…

Solar and Stellar Astrophysics · Physics 2015-06-17 Lucianne M. Walkowicz , Gibor S. Basri

We present an analysis of the starspot evolution, the surface differential rotation (SDR), the correlation between chromospheric activity indicators and the spatial connection between chromospheric and photospheric activities on the active…

Solar and Stellar Astrophysics · Physics 2021-01-11 Fukun Xu , Shenghong Gu , Panogiotis Ioannidis

We present results from a 5-month photometric survey for stellar rotation periods combined with a 4-year radial-velocity survey for membership and binarity in the 220Myr open cluster M34. We report surface rotation periods for 120 stars, 83…

Solar and Stellar Astrophysics · Physics 2015-05-27 Søren Meibom , Robert D. Mathieu , Keivan G. Stassun , Paul Liebesny , Steven H. Saar

We present an investigation of spin-orbit angles for planetary system candidates reported by Kepler. By combining the rotational period $P_s$ inferred from the flux variation due to starspots and the projected rotational velocity $V\sin…

Earth and Planetary Astrophysics · Physics 2015-06-05 Teruyuki Hirano , Roberto Sanchis-Ojeda , Yoichi Takeda , Norio Narita , Joshua N. Winn , Atsushi Taruya , Yasushi Suto

High-precision space-based photometry obtained by the \emph{Kepler} and \emph{TESS} missions has revealed evidence of rotational modulation associated with main sequence (MS) A and late-B type stars. Generally, such variability in these…

Solar and Stellar Astrophysics · Physics 2020-09-30 James Sikora , Gregg Wade , Jason Rowe

The field of the globular cluster M12 (NGC 6218) was monitored between 1995 and 2009 in a search for variable stars. $BV$ light curves were obtained for 36 periodic or likely periodic variables. Thirty-four of these are new detections.…

Solar and Stellar Astrophysics · Physics 2015-09-11 J. Kaluzny , I. B. Thompson , W. Narloch , W. Pych , M. Rozyczka

Stellar rotation is a fundamental ingredient in shaping the evolution of stars and it can also be used to trace past stellar interactions. Yet, systematic studies of stellar rotation in large samples of stars belonging to different…

The CoRoT space telescope observed nearly 160 000 light curves. Among the most outstanding is that of the young, active planet host star CoRoT-2A. In addition to deep planetary transits, the light curve of CoRoT-2A shows strong rotational…

Solar and Stellar Astrophysics · Physics 2016-05-25 Evangelos Nagel , Stefan Czesla , Jürgen H. M. M. Schmitt

We have developed a new method, K2, optimized for the detection of galaxy clusters in multicolor images. Based on the Red Sequence approach, K2 detects clusters using simultaneous enhancements in both colors and position. The detection…

Cosmology and Nongalactic Astrophysics · Physics 2014-11-20 Karun Thanjavur , Jon Willis , David Crampton

The stellar evolution theory of massive stars remains uncalibrated with high-precision photometric observational data mainly due to a small number of luminous stars that are monitored from space. Automated all-sky surveys have revealed…

Solar and Stellar Astrophysics · Physics 2017-02-08 Jaan Laur , Indrek Kolka , Tõnis Eenmäe , Taavi Tuvikene , Laurits Leedjärv

The extended Kepler mission (K2) has revealed more than 500 transiting planets in roughly 500,000 stellar light curves. All of these were found either with the box least-squares algorithm or by visual inspection. Here we use our new transit…

Earth and Planetary Astrophysics · Physics 2019-07-15 René Heller , Michael Hippke , Kai Rodenbeck
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