Model test for very-metal-poor giant
Nature Astronomy, Published online: 14 August 2024; doi:10.1038/s41550-024-02353-1 Model test for very-metal-poor giant ————— Free Secure Email – Transcom Sigma Transcom Hosting Transcom Premium Domains
Latest on LEO's & GEO's
Nature Astronomy, Published online: 14 August 2024; doi:10.1038/s41550-024-02353-1 Model test for very-metal-poor giant ————— Free Secure Email – Transcom Sigma Transcom Hosting Transcom Premium Domains
Nature Astronomy, Published online: 14 August 2024; doi:10.1038/s41550-024-02352-2 Magnetic field enhancement within a remnant ————— Free Secure Email – Transcom Sigma Transcom Hosting Transcom Premium Domains
Nature Astronomy, Published online: 12 August 2024; doi:10.1038/s41550-024-02337-1 How a star cluster manages to produce γ-rays at a location 30 light yr away from itself is a mystery that can be solved by carefully testing theories about how charged particles travel
Nature Astronomy, Published online: 07 August 2024; doi:10.1038/s41550-024-02336-2 Giant shock waves at the physical boundaries of the most massive structures in the Universe could be used as an accurate tool to measure the total mass of clusters of galaxies. —————
Nature Astronomy, Published online: 05 August 2024; doi:10.1038/s41550-024-02338-0 Merging supermassive black holes emit low-frequency gravitational waves, difficult to observe with current and future detectors. Stegmann et al. show that these black holes can leave measurable traces in high-frequency signals from
Nature Astronomy, Published online: 02 August 2024; doi:10.1038/s41550-024-02348-y Author Correction: Evidence for auroral influence on Jupiter’s nitrogen and oxygen chemistry revealed by ALMA ————— Free Secure Email – Transcom Sigma Transcom Hosting Transcom Premium Domains