№ files_lp_4_process_3_066441
Year: 2026
Region / Location: NGC 2287 (M 41), Milky Way
Subject: Stellar clusters, stellar rotation, magnetic activity
Document type: Research article
Institution: Rochester Institute of Technology, Chandra X-ray Center
Authors: Benjamin Ramsey, Joel Kastner, Ryan Butler, Alexander Binks, Tom Skillman
Target audience: Astrophysicists, astronomers
Observation period: Gaia DR3 release, TESS observations, recent Chandra HRC imaging
Data sources: Gaia Data Release 3, TESS, Chandra X-ray Observatory
Methodology: VR-assisted 3D kinematic analysis, light curve fitting, parallax and proper motion tests, color-magnitude diagram filtering
Funding: SAO grant G04-25013X
Preliminary results: Rotational bifurcation along upper main sequence, identification of rotational sequences in late-type stars, X-ray activity patterns
Research focus: Stellar structure, formation, and evolution analysis using cluster members
Peer review status: Not specified
Gaia DR3 data used: Yes
TESS data used: Yes
Chandra data used: Yes
Price: 8 / 10 USD
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