Nearby voids and their galaxies: recent progress and prospects
S. Pustilnik (1), Y. Perepelitsyna (1), A. Tepliakova (1), A.Kniazev, (1,2), E.Egorova (1,2), J. Chengalur (3), S.Kurapati (4) ((1) SAO RAS, (2), SAI MSU, (3) NCRA, Pune, (4) Department of Astronomy, University of Cape, Town, South Africa)

TL;DR
This paper reviews recent progress in studying nearby cosmic voids and their galaxies, highlighting findings on galaxy evolution, properties, and structure, and discusses future prospects with upcoming observational facilities.
Contribution
It provides a comprehensive overview of current void galaxy research, including new samples, key findings, and future directions in the field.
Findings
Void galaxies show signs of slower evolution.
Discovery of very metal-poor, gas-rich dwarf galaxies.
Clustering patterns relate to void substructures.
Abstract
Voids occupy about 3/4 of the volume of the Universe and contain about 15% of its mass. Due to various observational selection effects, these structure elements and galaxies populating voids, are highly under-explored. This especially relates to the lowest mass galaxies which comprise the main void population. Studying the nearby voids allows us to improve our understanding of the most elusive void objects. We present the brief overview of the current status and the prospects of the study of the nearest voids and their galaxies. First, we summarize the pioneer study of a hundred galaxies residing in the nearby Lynx-Cancer void which clearly evidence for the slower evolution of void galaxies and finds also the unusual very metal-poor and gas-rich dwarfs. Then we describe the recently defined sample of the nearby voids within the sphere with R = 25 Mpc and a sample of 1350 galaxies…
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Taxonomy
TopicsAstronomy and Astrophysical Research · Galaxies: Formation, Evolution, Phenomena · Adaptive optics and wavefront sensing
