Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF PPT Format

A Noninteracting Galactic Black Hole Candidate in a Binary System with a Main-sequence Star

  • Authors: Sukanya Chakrabarti, Joshua D. Simon, Peter A. Craig, Henrique Reggiani, Timothy D. Brandt, Puragra Guhathakurta, Paul A. Dalba, Evan N. Kirby, Philip Chang, Daniel R. Hey, Alessandro Savino, Marla Geha, Ian B. Thompson

Sukanya Chakrabarti et al 2023 The Astronomical Journal 166 .

  • Provider: AAS Journals

Caption: Figure 10.

MCMC results for the orbital solution determined from the radial velocity data listed in Table 2, showing only elements in the chain with periods between 175 and 195 days. Although some of the parameters exhibit significant correlations, the overall orbital properties are well constrained by the data, with results similar to those expected from the astrometric solution. Some parameters, such as K 1, do have significant uncertainties.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article

Show More

Copyright and Terms & Conditions

Additional terms of reuse