Blue Large-Amplitude Pulsators and Other Short-Period Variable Stars in OGLE-IV Fields of the Outer Galactic Bulge
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| Main Authors: | , , , , , , , , , , , , , , , |
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| Format: | Preprint |
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2024
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| author | Borowicz, J. Pietrukowicz, P. Skowron, J. Soszyński, I. Udalski, A. Szymański, M. K. Ulaczyk, K. Poleski, R. Kozłowski, S. Mróz, P. Skowron, D. M. Rybicki, K. Iwanek, P. Wrona, M. Gromadzki, M. Mróz, M. J. |
| author_facet | Borowicz, J. Pietrukowicz, P. Skowron, J. Soszyński, I. Udalski, A. Szymański, M. K. Ulaczyk, K. Poleski, R. Kozłowski, S. Mróz, P. Skowron, D. M. Rybicki, K. Iwanek, P. Wrona, M. Gromadzki, M. Mróz, M. J. |
| contents | In this work, we search the OGLE-IV outer Galactic bulge fields for short-period variable objects. The investigation focuses on unexplored timescales roughly below one hour in an area containing about 700 million stellar sources down to approximately I=20 mag. We concentrate mainly on Blue Large-Amplitude Pulsators (BLAPs), which represent a recently discovered enigmatic class of short-period hot subluminous stars. We find 33 BLAPs in the period range from 7.5 to 66.5 min. Thirty-one of them are new discoveries, which increases the number of known stars of this class to over one hundred. Additional eighteen objects with pulsation-like light curve shapes and periods ranging from 17.3 to 53.7 min are presented. Very likely, these are $δ$ Sct/SX Phe-type stars, but some of them could be pulsating hot subdwarfs or BLAPs. We also report on the detection of five eclipsing binary systems with orbital periods between 61.2 and 121.9 min and three mysterious variable objects with I-band amplitudes larger than 0.9 mag. A spectroscopic follow-up would help in the final classification of the variables. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2404_17715 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Blue Large-Amplitude Pulsators and Other Short-Period Variable Stars in OGLE-IV Fields of the Outer Galactic Bulge Borowicz, J. Pietrukowicz, P. Skowron, J. Soszyński, I. Udalski, A. Szymański, M. K. Ulaczyk, K. Poleski, R. Kozłowski, S. Mróz, P. Skowron, D. M. Rybicki, K. Iwanek, P. Wrona, M. Gromadzki, M. Mróz, M. J. Solar and Stellar Astrophysics In this work, we search the OGLE-IV outer Galactic bulge fields for short-period variable objects. The investigation focuses on unexplored timescales roughly below one hour in an area containing about 700 million stellar sources down to approximately I=20 mag. We concentrate mainly on Blue Large-Amplitude Pulsators (BLAPs), which represent a recently discovered enigmatic class of short-period hot subluminous stars. We find 33 BLAPs in the period range from 7.5 to 66.5 min. Thirty-one of them are new discoveries, which increases the number of known stars of this class to over one hundred. Additional eighteen objects with pulsation-like light curve shapes and periods ranging from 17.3 to 53.7 min are presented. Very likely, these are $δ$ Sct/SX Phe-type stars, but some of them could be pulsating hot subdwarfs or BLAPs. We also report on the detection of five eclipsing binary systems with orbital periods between 61.2 and 121.9 min and three mysterious variable objects with I-band amplitudes larger than 0.9 mag. A spectroscopic follow-up would help in the final classification of the variables. |
| title | Blue Large-Amplitude Pulsators and Other Short-Period Variable Stars in OGLE-IV Fields of the Outer Galactic Bulge |
| topic | Solar and Stellar Astrophysics |
| url | https://arxiv.org/abs/2404.17715 |