Molecular gas content of shell galaxies

Shells are fine stellar structures that are identified by their arc-like shapes around a galaxy. They are currently thought to be vestiges of galaxy interactions and/or mergers. The study of their number, geometry, stellar populations, and gas content can help us to derive the interaction or merger...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2019-10, Vol.630, p.A112
Hauptverfasser:	Mancillas, B., Combes, F., Duc, P.-A.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Clumps Galactic Astrophysics Galactic rotation galaxies: interactions galaxies: ISM galaxies: kinematics and dynamics galaxies: peculiar galaxies: structure Molecular gases Neutral gases Radial velocity Sciences of the Universe Shell galaxies Spatial resolution Stars & galaxies Stellar populations
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