Hidden in Plain Sight: Searching for Dark Companions to Bright Stars with the Large Binocular Telescope and SHARK-VIS

March 2025 • 2025ApJ...981...94R

Authors • Rowan, D. M. • Thompson, T. A. • Kochanek, C. S. • Li Causi, G. • Roth, J. • Vaccari, P. • Pedichini, F. • Piazzesi, R. • Antoniucci, S. • Testa, V. • Johnson, M. C. • Crass, J. • Crepp, J. R. • Bechter, A. • Bechter, E. B. • Sands, B. L. • Harris, R. J. • Fulton, B. J.

Abstract • We report the results from a pilot study to search for black holes and other dark companions in binary systems using direct imaging with SHARK-VIS and the iLocater pathfinder "Lili" on the Large Binocular Telescope. Starting from known single-lined spectroscopic binaries, we select systems with high mass functions that could host dark companions and whose spectroscopic orbits indicate a projected orbital separation ≥30 mas. For this first exploration, we selected four systems (HD 137909, HD 104438, HD 117044, and HD 176695). In each case, we identify a luminous companion and measure the flux ratio and angular separation. However, two of the systems (HD 104438 and HD 176695) are not consistent with simple binary systems and are most likely hierarchical triples. The observed companions rule out a massive compact object for HD 137909, HD 117044, and HD 176695. HD 104438 requires further study because the identified star cannot be responsible for the RV orbit and is likely a dwarf tertiary companion. The SHARK-VIS observation was taken near pericenter, and a second image near apocenter is needed to discriminate between a closely separated luminous secondary and a compact object. When a luminous companion is found, the combination of the RVs and the single SHARK-VIS observation strongly constrains the orbital inclination and the companion mass. Since a single SHARK-VIS observation has a typical on-source observing time of only ∼10 minutes, this a promising method to efficiently identify non-interacting compact object candidates.

Links

• PDF https://iopscience.iop.org/article/10.3847/1538-4357/adad6e/pdf
• ELECTR https://iopscience.iop.org/article/10.3847/1538-4357/adad6e
• PREPRINT http://arxiv.org/abs/2410.19050