What goes around comes around: The fate of stars in stripped tails of gas
We conducted high-resolution wind-tunnel simulations to study in situ star formation in the stripped tails of two massive ( M star = 10 11 M ⊙ ) galaxies undergoing time-evolving ram pressure stripping. One galaxy was stripped face-on (W0), and the other was subject to an angled wind (W45). We find...
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Published in | Astronomy and astrophysics (Berlin) Vol. 698; p. A151 |
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Main Authors | , , , , , , , |
Format | Journal Article |
Language | English |
Published |
01.06.2025
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Online Access | Get full text |
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