Deciphering Lyman-α emission deep into the epoch of reionization

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Nature Astronomy, Published online: 18 January 2024; doi:10.1038/s41550-023-02179-3

A combination of JWST/NIRCam observations and magnetohydrodynamic simulations indicates that frequent mergers with close companions give rise to bursty star formation and hence the unexpectedly high Lyman-α emission detected from early galaxies.

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Deciphering Lyman-α emission deep into the epoch of reionization

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The nested morphology of disk winds from young stars revealed by JWST/NIRSpec observations

We may be looking for Martian life in the wrong place

Universal bimodality in kinematic morphology and the divergent pathways to galaxy quenching

Follow the serpentine as a comprehensive diagnostic for extraterrestrial habitability

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