Analysis of the Multuple Star System WDS 08375-3345 HJ 4115
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This is a updated version of this paper previously submitted Feb 23rd. I had received a late reply from a colleague with comments. My apologies to the reviewer if the paper has already been reviewed.Abstract
The multiple star system WDS 08375-3345 HJ 4115 is analyzed using new data from the Gaia DR3 catalog. The Gaia parallaxes show the A and B components in close proximity to the Sun at 60.4 parsecs distance. Astrometric, photometric and other data are combined to determine if the system forms a gravitationally bound binary star system.
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Published
2025-04-05
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