Verification of Hypervelocity Bulge Red Clump Stars

Fuente: arXiv
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Main Authors: Wojtkowska, Gabriela, Poleski, Radosław
Format: Preprint
Published: 2024
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author Wojtkowska, Gabriela
Poleski, Radosław
author_facet Wojtkowska, Gabriela
Poleski, Radosław
contents We verify candidate hypervelocity red clump stars located in the Galactic bulge that were selected based on the VVV and the Gaia DR2 data by Luna et al. (2019). To do so, we analyze data from the OGLE-IV survey: difference images and astrometric time series. We have data for 30 stars out of 34 hypervelocity candidates. We confirmed high proper motion of only one of these stars and find out that it is a nearby one, hence, not hypervelocity. To sum up, we do not confirm the candidate stars as hypervelocity ones. Hence, we disprove the production rate of hypervelocity red clump stars by the central supermassive black hole provided by Luna et al. (2019).
format Preprint
id arxiv_https___arxiv_org_abs_2403_03311
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Verification of Hypervelocity Bulge Red Clump Stars
Wojtkowska, Gabriela
Poleski, Radosław
Solar and Stellar Astrophysics
Astrophysics of Galaxies
We verify candidate hypervelocity red clump stars located in the Galactic bulge that were selected based on the VVV and the Gaia DR2 data by Luna et al. (2019). To do so, we analyze data from the OGLE-IV survey: difference images and astrometric time series. We have data for 30 stars out of 34 hypervelocity candidates. We confirmed high proper motion of only one of these stars and find out that it is a nearby one, hence, not hypervelocity. To sum up, we do not confirm the candidate stars as hypervelocity ones. Hence, we disprove the production rate of hypervelocity red clump stars by the central supermassive black hole provided by Luna et al. (2019).
title Verification of Hypervelocity Bulge Red Clump Stars
topic Solar and Stellar Astrophysics
Astrophysics of Galaxies
url https://arxiv.org/abs/2403.03311