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机译:The nature of the 2014-2015 dim state of RW Aurigae revealed by X-ray, optical, and near-IR observations
European Space Res & Technol Ctr ESA ESTEC, NL-2201 AZ Noordwijk, Netherlands;
MIT, Kavli Inst Astrophys & Space Res, Cambridge, MA 02139 USA;
Hamburger Sternwarte, D-21029 Hamburg, GermanyUniv Cambridge, Inst Astron, Cambridge CB3 0HA, EnglandInst Astron, Hilo, HI 96720 USAUniv Colorado, Boulder, CO 80309 USAHarvard Smithsonian Ctr Astrophys, Cambridge, MA 02139 USA;
stars: individual: RW Aur; stars: pre-main sequence; stars: low-mass; stars: variables: T Tauri; Herbig Ae/Be; X-rays: stars;