Extremely metal poor (XMP) galaxies are the least chemically evolved objects in the local Universe and provide important constraints on galaxy formation in low-metallicity environments. This work investigates the ionised gas kinematics and star formation properties of XMP galaxies to identify signatures of disturbed or...
J. Yadav, C. Muñoz-Tuñón, Cecilia Fariña et al.· Astronomy & Astrophysics· 0 citations
Extremely Metal Poor (XMP) galaxies are the least chemically evolved objects in the local Universe and provide important constraints on galaxy formation in low-metallicity environments. This work investigates the ionised gas kinematics and star formation properties of XMP galaxies to identify disturbed or multi-compone...
J. Yadav, C. M. Tuñón, Cecilia Fariña et al.· 0 citations
Understanding how stars form at low metallicity is challenging because the usual probe of the molecular gas reservoir, carbon monoxide (CO) emission, is faint, and tends to be concentrated in parsec-scale clumps. To overcome this difficulty in our study of molecular clouds in metal-poor environments, we have acquired ̧...
L. Hunt, M. Heyer, U. Lisenfeld et al.· Astronomy & Astrophysics· 0 citations
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