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200 papers

The effect of light refraction in a galaxy halo of dark matter, described by profiles of Navarro-Frenk-White and Burkett, was considered. Powers of the Cherenkov radiation for the refractive indexes of gravitational fields with these…

Cosmology and Nongalactic Astrophysics · Physics 2013-02-18 Leonid M Chechin

The Blazhko effect in CX Lyr has been reported for the first time by Le Borgne et al. (2007). The authors have pointed out that the Blazhko period was not evaluated accurately due to dataset scarcity. The possible period values announced…

Solar and Stellar Astrophysics · Physics 2012-12-04 Pierre de Ponthiere , Jean-Francois Le Borgne , Franz-Josef Hambsch

The simultaneous photometric and spectroscopic observations of the RR Lyrae variables in the globular cluster, M3, published in Jurcsik et al. (2017, Paper I) made it possible to perform Baade-Wesselink (BW) analysis of a large sample of…

Solar and Stellar Astrophysics · Physics 2017-07-26 J. Jurcsik , G. Hajdu

This is a brief overview of the elemental abundance patterns that have been observed in the different Galactic stellar populations. Main focus is on studies that are based on high-resolution spectra of dwarf and subgiant stars, and in some…

Astrophysics of Galaxies · Physics 2013-12-18 Thomas Bensby

The Galactic O-Star Spectroscopic Survey (GOSSS) is obtaining high quality R~2500 blue-violet spectroscopy of all Galactic stars ever classified as of O type with B < 12 and a significant fraction of those with B = 12-14. As of June 2013,…

Blazars, a type of active galactic nuclei (AGN) with relativistic jets pointed at the observer, exhibit flux variability across the electromagnetic spectrum due to particle acceleration in their jets. Power spectral density (PSD) studies…

We report the results of an observational study aimed at searching for magnetic pulsating hot stars suitable for magneto-asteroseismology. A sample of sixteen chemically peculiar stars was selected and analysed using both high-resolution…

Solar and Stellar Astrophysics · Physics 2018-07-04 B. Buysschaert , C. Neiner , A. J. Martin , C. Aerts , D. M. Bowman , M. E. Oksala , T. Van Reeth

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…

Solar and Stellar Astrophysics · Physics 2014-06-18 M. Skarka , M. Zejda

A photometric survey of three Southern target fields with BEST II yielded the detection of 2,406 previously unknown variable stars and an additional 617 stars with suspected variability. This study presents a catalog including their…

The stellar parameters of RR Lyrae stars vary considerably over a pulsation cycle, and their determination is crucial for stellar modelling. We present a detailed spectroscopic analysis of the pulsating star RR Lyr, the prototype of its…

Solar and Stellar Astrophysics · Physics 2015-06-23 L. Fossati , K. Kolenberg , D. V. Shulyak , A. Elmasli , V. Tsymbal , T. G. Barnes , E. Guggenberger , O. Kochukhov

Red clump giants in the Galactic bulge are approximate standard candles and hence they can be used as distance indicators. We compute the proper motion dispersions of RCG stars in the Galactic bulge using the proper motion catalogue from…

We have conducted a spectroscopic analysis of the bulges of a sample of 31 spiral galaxies, spanning the Hubble sequence from S0 to Scd type, in order to study the radial distribution of their stellar population properties.

Astrophysics · Physics 2009-11-07 P. Jablonka , J. Gorgas , P. Goudfrooij

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 present the results of a photometry campaign of TU Com performed over a five-year time span. The analysis showed that the possible Blazhko period of 75 days published by the General Catalogue of Variable Stars is not correct. We…

Solar and Stellar Astrophysics · Physics 2016-05-12 Pierre de Ponthiere , Franz-Josef Hambsch , Kenneth Menzies , Richard Sabo

The results presented are a continuation of observing campaigns conducted by a small group of amateur astronomers interested in the Blazhko effect of RR Lyrae stars. The goal of these observations is to confirm the RR Lyrae Blazhko effect…

Solar and Stellar Astrophysics · Physics 2014-07-17 Pierre de Ponthiere , Franz-Josef , Hambsch , Kenneth Menzies , Richard Sabo

I review the properties of the Galaxy's stellar halo, specifically as traced by horizontal branch stars, but with reference to and in comparison with other stellar tracers. I discuss the halo density profile, the variation in horizontal…

Astrophysics · Physics 2007-05-23 Andrew C. Layden

We initiated digitization of the Moscow collection of astronomical plates using flatbed scanners. Techniques of photographic photometry of the digital images were applied, enabling an effective search for new variable stars. Our search for…

Astrophysics · Physics 2008-10-08 D. M. Kolesnikova , L. A. Sat , K. V. Sokolovsky , S. V. Antipin , N. N. Samus

Context. The Blazhko effect, in RR Lyrae type stars, is a century old mystery. Dozens of theory exists, but none have been able to entirely reproduce the observational facts associated to this modulation phenomenon. Existing theory all rely…

Solar and Stellar Astrophysics · Physics 2016-10-25 Cyrus Zalian

We present a catalog of over 6.2 million stars with measured proper motions. All these stars are observed in the direction of the Magellanic Clouds within the brightness range 12 < I < 19 mag. Based on these proper motions about 440 000…

Astrophysics of Galaxies · Physics 2012-04-26 R. Poleski , I. Soszyński , A. Udalski , M. K. Szymański , M. Kubiak , G. Pietrzyński , Ł. Wyrzykowski , K. Ulaczyk

We report the detection of 45 candidate microlensing events in fields toward the Galactic bulge. These come from the analysis of 24 fields containing 12.6 million stars observed for 190 days in 1993. Many of these events are of extremely…