Blue Large-Amplitude Pulsators and Other Short-Period Variable Stars in the OGLE-IV Galactic Disk Fields

Fuente: arXiv
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Auteurs principaux: Borowicz, J., Pietrukowicz, P., Mróz, P., Soszyński, I., Udalski, A., Szymański, M. K., Ulaczyk, K., Poleski, R., Kozłowski, S., Skowron, J., Skowron, D. M., Rybicki, K., Iwanek, P., Wrona, M., Gromadzki, M.
Format: Preprint
Publié: 2023
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author Borowicz, J.
Pietrukowicz, P.
Mróz, P.
Soszyński, I.
Udalski, A.
Szymański, M. K.
Ulaczyk, K.
Poleski, R.
Kozłowski, S.
Skowron, J.
Skowron, D. M.
Rybicki, K.
Iwanek, P.
Wrona, M.
Gromadzki, M.
author_facet Borowicz, J.
Pietrukowicz, P.
Mróz, P.
Soszyński, I.
Udalski, A.
Szymański, M. K.
Ulaczyk, K.
Poleski, R.
Kozłowski, S.
Skowron, J.
Skowron, D. M.
Rybicki, K.
Iwanek, P.
Wrona, M.
Gromadzki, M.
contents Blue Large-Amplitude Pulsators (BLAPs) form a mysterious class of variable stars with typical periods of tens of minutes and amplitudes above 0.1 mag. In this work, we present results of a variability search focused on timescales shorter than 1 h, conducted in OGLE-IV Galactic disk fields containing about 1.1 billion stellar sources down to I$\approx$20 mag. Twenty-five BLAPs have been detected, 20 of which are new discoveries. Their periods range from 8.4 min to 62.1 min. We have also found six new eclipsing binary systems with orbital periods from 38.3 min to 121.3 min and five short-period large-amplitude (> 0.17 mag in the I-band) variable stars of unknown type.
format Preprint
id arxiv_https___arxiv_org_abs_2309_06012
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Blue Large-Amplitude Pulsators and Other Short-Period Variable Stars in the OGLE-IV Galactic Disk Fields
Borowicz, J.
Pietrukowicz, P.
Mróz, P.
Soszyński, I.
Udalski, A.
Szymański, M. K.
Ulaczyk, K.
Poleski, R.
Kozłowski, S.
Skowron, J.
Skowron, D. M.
Rybicki, K.
Iwanek, P.
Wrona, M.
Gromadzki, M.
Solar and Stellar Astrophysics
Astrophysics of Galaxies
Blue Large-Amplitude Pulsators (BLAPs) form a mysterious class of variable stars with typical periods of tens of minutes and amplitudes above 0.1 mag. In this work, we present results of a variability search focused on timescales shorter than 1 h, conducted in OGLE-IV Galactic disk fields containing about 1.1 billion stellar sources down to I$\approx$20 mag. Twenty-five BLAPs have been detected, 20 of which are new discoveries. Their periods range from 8.4 min to 62.1 min. We have also found six new eclipsing binary systems with orbital periods from 38.3 min to 121.3 min and five short-period large-amplitude (> 0.17 mag in the I-band) variable stars of unknown type.
title Blue Large-Amplitude Pulsators and Other Short-Period Variable Stars in the OGLE-IV Galactic Disk Fields
topic Solar and Stellar Astrophysics
Astrophysics of Galaxies
url https://arxiv.org/abs/2309.06012