Giant low surface brightness disc galaxies (gLSBs) are rare objects with disc radii up to 130 kpc and total masses of 10^12 solar masses. They challenge currently accepted theories of galaxy formation and evolution, because it is difficult to build-up such large dynamically cold systems via mergers while preserving such extended discs. Recently we significantly extended a sample of gLSB galaxies by visual inspecting of 120 sq. deg. covered by deep Hyper Suprime-Cam data and found 42 new gLSB systems (Saburova et al. 2022). Here we propose a pilot HI observations of 4 gLSBs aiming to determine their neutral atomic hydrogen gas content and dark matter fraction derived from the rotation of the galaxies.
Name | Institution |
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Philip Lah * | Abu Dhabi, New York University |
Joseph Gelfand | New York University; National Science Foundation ; Abu Dhabi, New York University |
Ivan Katkov | Abu Dhabi, New York University |
* indicates the PI