Hα as a tracer of star formation in the SPHINX cosmological simulations
The Hα emission line in galaxies is a powerful tracer of their recent star formation activity. With the advent of JWST, we are now able to routinely observe Hα in galaxies at high redshift (z ≳ 3) and thus measure their star formation rates (SFRs). However, using classical SFR(Hα) calibrations to de...
Αποθηκεύτηκε σε:
| Κύριοι συγγραφείς: | , , , , , |
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| Μορφή: | Artigo |
| Γλώσσα: | Inglês |
| Έκδοση: |
EDP Sciences
2026-03-01
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| Σειρά: | Astronomy & Astrophysics |
| Θέματα: | |
| Διαθέσιμο Online: | https://www.aanda.org/articles/aa/full_html/2026/03/aa57114-25/aa57114-25.html |
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