Nature Astronomy, Published online: 08 April 2024; doi:10.1038/s41550-024-02244-5 A state-of-the-art simulation reveals that the long-lasting 10 MK plasma in solar active regions can be heated by magnetic reconnections driven by continuous flux emergence that repeatedly deposit impulsive heating into the coronal

Nature Astronomy, Published online: 08 April 2024; doi:10.1038/s41550-024-02225-8 Radio pulses from a rare, radio-loud magnetar, XTE J1810−197, are seen to have undergone a conversion in their polarization state. This change can be linked to the magnetar’s magnetic field geometry, and

Nature Astronomy, Published online: 08 April 2024; doi:10.1038/s41550-024-02226-7 A radio-loud magnetar, XTE J1810–197, has been observed to precess shortly after an X-ray outburst. The precession decayed over the subsequent few months, which probably rules out freely precessing magnetars as the source

Nature Astronomy, Published online: 26 March 2024; doi:10.1038/s41550-024-02229-4 Micrometeorite impacts are an important process in forming several Ti oxides, including rutile (TiO2) and new Ti minerals (trigonal Ti2O and triclinic Ti2O). These Ti oxides can alter the photocatalytic properties and

Nature Astronomy, Published online: 20 March 2024; doi:10.1038/s41550-024-02234-7 Rapidly rotating or not? ————— Free Secure Email – Transcom Sigma Transcom Hosting Transcom Premium Domains

Nature Astronomy, Published online: 20 March 2024; doi:10.1038/s41550-024-02235-6 TheCannon for abundances in solar analogues ————— Free Secure Email – Transcom Sigma Transcom Hosting Transcom Premium Domains