Hostname: page-component-586b7cd67f-rdxmf Total loading time: 0 Render date: 2024-11-23T20:49:03.579Z Has data issue: false hasContentIssue false
  • English
  • Français

Hunting for massive binaries with a black-hole component using Gaia data

Published online by Cambridge University Press:  29 August 2024

Soetkin Janssens Open the ORCID record for Soetkin Janssens [Opens in a new window] ,
T. Shenar Open the ORCID record for T. Shenar [Opens in a new window] ,
H. Sana Open the ORCID record for H. Sana [Opens in a new window] ,
S. Faigler ,
N. Langer Open the ORCID record for N. Langer [Opens in a new window] ,
P. Marchant ,
T. Mazeh ,
C. Schürmann Open the ORCID record for C. Schürmann [Opens in a new window]  and
S. Shahaf
Soetkin Janssens*
Affiliation:
Institute of Astronomy, KU Leuven, Celestijnenlaan 200D, 3001 Leuven, Belgium
T. Shenar
Affiliation:
Anton Pannekoek Institute for Astronomy, Science Park 904, 1098 XH, Amsterdam, The Netherlands
H. Sana
Affiliation:
Institute of Astronomy, KU Leuven, Celestijnenlaan 200D, 3001 Leuven, Belgium
S. Faigler
Affiliation:
School of Physics and Astronomy, Tel Aviv University, Tel Aviv 6997801, Israel
N. Langer
Affiliation:
Argelander-Institut für Astronomie, Universität Bonn, Auf dem Hügel 71, 53121 Bonn, Germany Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
P. Marchant
Affiliation:
Institute of Astronomy, KU Leuven, Celestijnenlaan 200D, 3001 Leuven, Belgium
T. Mazeh
Affiliation:
School of Physics and Astronomy, Tel Aviv University, Tel Aviv 6997801, Israel
C. Schürmann
Affiliation:
Argelander-Institut für Astronomie, Universität Bonn, Auf dem Hügel 71, 53121 Bonn, Germany Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
S. Shahaf
Affiliation:
Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot 7610001, Israel
*
email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

With the upcoming third Gaia data release (DR3), the first Gaia astrometric orbital solutions for binary sources will become available. Potentially, many rarely seen single-degenerate massive binaries with a black hole (OB+BH) will be revealed. Here, we investigate how many OB+BHs are expected to be detected as binaries in Gaia astrometry by using tailored models for the massive star population. We use a method based on the astrometric data to investigate how many OB+BH binaries will be uncovered by Gaia. We estimate that∼200 OB+BHs are detectable among the sources in the second Alma Luminous Star massive star catalogue, either in DR3 or in upcoming data releases. Moreover, we show that BH-formation scenarios could be constrained from the distributions of parameters such as the orbital periods and eccentricities.

Keywords

black hole physicsbinaries:generalastrometrystars:statistics
Type
Poster Paper
Information
Proceedings of the International Astronomical Union , Volume 18 , Symposium S361: Massive Stars Near and Far , May 2022 , pp. 313 - 315
Check for updates
Copyright
© The Author(s), 2024. Published by Cambridge University Press on behalf of International Astronomical Union

References

Abdul-Masih, M., et al. 2020, Nature, 580, E11 Google Scholar
Bodensteiner, J., et al. 2020, A&A, 641, A43 Google Scholar
Casares, J., Negueruela, I., Ribó, M., Ribas, I., Paredes, J. M., Herrero, A., & Simón-Daz, S. 2014, Nature, 505, 378 CrossRefGoogle Scholar
Corral-Santana, J. M., Casares, J., Muñoz-Darias, T., Bauer, F. E., Martnez-Pais, I. G., & Russell, D. M. 2016, A&A, 587, A61 Google Scholar
El-Badry, K., & Quataert, E. 2020, MNRAS, 493, L22 CrossRefGoogle Scholar
Frost, A. J., et al. 2022, A&A, 659, L3 CrossRefGoogle Scholar
Irrgang, A., Geier, S., Kreuzer, S., Pelisoli, I., & Heber, U. 2020, A&A, 633, L5 CrossRefGoogle Scholar
Janssens, S., et al. 2022, A&A, 658, A129 Google Scholar
Langer, N., et al. 2020, A&A, 638, A39 Google Scholar
Mahy, L., et al. 2022, arXiv e-prints, arXiv:2207.07752Google Scholar
Mazeh, T., & Faigler, S. 2020, MNRAS, 498, L58 CrossRefGoogle Scholar
Pantaleoni González, M., Maz Apellániz, J., Barbá, R. H., & Reed, B. C. 2021, MNRAS, 504, 2968 Google Scholar
Sana, H., et al. 2012, Science, 337, 444 CrossRefGoogle Scholar
Shahaf, S., Mazeh, T., Faigler, S., & Holl, B. 2019, MNRAS, 487, 5610 CrossRefGoogle Scholar
Shenar, T., et al. 2020, A&A, 639, L6 Google Scholar
Shenar, T.. 2022, Nature AstronomyGoogle Scholar