An HST survey of photometry and multiplicity of brown dwarfs and planetary-mass objects in the field of Taurus
astro-ph.SR, astro-ph.EP
Submitted: 2026-10-15
Updated: 2026-10-15
Comments: 19 pages, 10 figures, accepted for publication in MNRAS
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Sources
- Multiplicity of young isolated planetary mass objects in Taurus and Upper Scorpius
- The SpeX Prism Library: 1000+ Low-resolution, Near-infrared Spectra of Ultracool M, L, T and Y Dwarfs
- Not Alone: Tracing the Origins of Very Low Mass Stars and Brown Dwarfs Through Multiplicity Studies
- The Pan-STARRS1 Surveys
- The Montreal Open Clusters and Associations (MOCA) Database: A Census of Nearby Associations, Open Clusters, and Young Substellar Objects within 500 pc of the Sun
- Low Mass Star Formation in the Taurus-Auriga Clouds
- The Origin and Evolution of Multiple Star Systems
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