The OGLE Collection of Variable Stars: Over 18 000 Rotating Variables toward the Galactic Bulge
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| Main Authors: | , , , , , , , , , , , , , , , , |
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| Format: | Preprint |
| Published: |
2024
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| _version_ | 1866916303519875072 |
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| author | Iwanek, P. Soszyński, I. Stępień, K. Kozłowski, S. Skowron, J. Udalski, A. Szymański, M. K. Wrona, M. Pietrukowicz, P. Poleski, R. Mróz, P. Ulaczyk, K. Skowron, D. M. Gromadzki, M. Rybicki, K. Mróz, M. J. Ratajczak, M. |
| author_facet | Iwanek, P. Soszyński, I. Stępień, K. Kozłowski, S. Skowron, J. Udalski, A. Szymański, M. K. Wrona, M. Pietrukowicz, P. Poleski, R. Mróz, P. Ulaczyk, K. Skowron, D. M. Gromadzki, M. Rybicki, K. Mróz, M. J. Ratajczak, M. |
| contents | Stellar rotation, a key factor influencing stellar structure and evolution, also drives magnetic activity, which is manifested as spots or flares on stellar surface. Here, we present a collection of 18 443 rotating variables located toward the Galactic bulge, identified in the photometric database of the Optical Gravitational Lensing Experiment (OGLE) project. These stars exhibit distinct magnetic activity, including starspots and flares. With this collection, we provide long-term, time-series photometry in Cousins I- and Johnson V-band obtained by OGLE since 1997, and basic observational parameters, i.e., equatorial coordinates, rotation periods, mean brightness, and brightness amplitudes in both bands. This is a unique dataset for studying stellar magnetic activity, including activity cycles. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2406_18728 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | The OGLE Collection of Variable Stars: Over 18 000 Rotating Variables toward the Galactic Bulge Iwanek, P. Soszyński, I. Stępień, K. Kozłowski, S. Skowron, J. Udalski, A. Szymański, M. K. Wrona, M. Pietrukowicz, P. Poleski, R. Mróz, P. Ulaczyk, K. Skowron, D. M. Gromadzki, M. Rybicki, K. Mróz, M. J. Ratajczak, M. Solar and Stellar Astrophysics Astrophysics of Galaxies Stellar rotation, a key factor influencing stellar structure and evolution, also drives magnetic activity, which is manifested as spots or flares on stellar surface. Here, we present a collection of 18 443 rotating variables located toward the Galactic bulge, identified in the photometric database of the Optical Gravitational Lensing Experiment (OGLE) project. These stars exhibit distinct magnetic activity, including starspots and flares. With this collection, we provide long-term, time-series photometry in Cousins I- and Johnson V-band obtained by OGLE since 1997, and basic observational parameters, i.e., equatorial coordinates, rotation periods, mean brightness, and brightness amplitudes in both bands. This is a unique dataset for studying stellar magnetic activity, including activity cycles. |
| title | The OGLE Collection of Variable Stars: Over 18 000 Rotating Variables toward the Galactic Bulge |
| topic | Solar and Stellar Astrophysics Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2406.18728 |