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BLACK_MELODY

BLACK holes MEasured and/or LOcated by DYnamical (radial velocity) method.

This repository will be updated every month, with a probability of 0.25.

Contents

About

This is a project aiming to collect stellar-mass black holes (BH) measured by the dynamical method. We have currently collected seven targets discovered in recent years and hopefully, the number will boost in a near future. To construct and study an unbiased mass distribution of Galactic stellar-mass BHs, one has to build a decent catalog of BHs discovered by different methods. Notably, BlackCat is "a thorough and comprehensive catalogue containing the most updated information about stellar-mass black holes (BHs), mainly focused in systems detected as X-ray transients." Our project is inspired by the fantastic work of Corral-Santana et al. 2016, but focuses on the dynamically discovered, X-ray quiet (or non-accreting) black holes. If I missed your dynamically discovered BH(s), please let me know immediately. Apologize for my ignorance!

Catalog Today

Here are seven BHs collected so far:

  • MW C656: Casares et al. 2014; A Be-type star with a black-hole companion
  • LB-1: Liu et al. 2019; A wide star-black-hole binary system from radial-velocity measurements
    and Liu et al. 2020; Phase-dependent Study of Near-infrared Disk Emission Lines in LB-1
  • 2MASS J05215658+4359220: Thompson et al. 2019; A noninteracting low-mass black hole–giant star binary system
  • HR 6819: Rivinius et al. 2021; A naked-eye triple system with a nonaccreting black hole in the inner binary
  • V723 Mon: Jayasinghe et al. 2021; A unicorn in monoceros: the 3 M⊙ dark companion to the bright, nearby red giant V723 Mon is a non-interacting, mass-gap black hole candidate
  • NGC 1850 BH1: Saracino et al. 2021; A black hole detected in the young massive LMC cluster NGC 1850
  • NGC2004#115: Lennon et al. 2021; The VLT-FLAMES survey of massive stars. NGC2004#115: A triple system hosting a possible short period B+BH binary

Note that some of them are candidates, great discussions on these systems have been carried out. See this ads library for follow-up papers that discuss these systems. As you can see, some of them may not actually contain a BH, but systems with tricky properties that confuse us and thus 'disguise' them as a BH. Surely, to discover and confirm a BH is not a trivial task, but that is all the fun in it!

Join the Project Now

If you would like to join my project, please just let me know. Your participations are most welcomed!

Maintainers

[email protected]

Change Log

black_melody's People

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