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Nearby void dwarf galaxies: recent results, the ongoing project and prospects

Published online by Cambridge University Press:  30 October 2019

Simon A. Pustilnik ,
Dmitri I. Makarov  and
Arina L. Tepliakova
Simon A. Pustilnik
Affiliation:
Special Astrophysical Observatory of RAS, 369167, Nizhnij Arkhyz, Karachai-Circessia, Russia emails: [email protected], [email protected]
Dmitri I. Makarov
Affiliation:
Special Astrophysical Observatory of RAS, 369167, Nizhnij Arkhyz, Karachai-Circessia, Russia emails: [email protected], [email protected]
Arina L. Tepliakova
Affiliation:
Special Astrophysical Observatory of RAS, 369167, Nizhnij Arkhyz, Karachai-Circessia, Russia emails: [email protected], [email protected]
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Abstract

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Properties of dwarf galaxies formed and evolved in the lowest density environment remain largely unexplored and poorly understood. Especially this concerns the low-mass end (Mbar < 109M⊙). We overview the results of systematic study of a hundred void dwarfs from the nearby Lynx-Cancer void. We describe the ongoing project aiming to form Nearby Void galaxy sample (R < 25 Mpc) over the whole sky. 1354 objects with distances less than 25 Mpc fall within 25 voids delineated by 460 luminous galaxies/groups. The void major sizes range from 13 to 37 Mpc. 1088 of 1354 void galaxies reside deeply in voids, having distances to the nearest luminous neighbour of 2–11 Mpc. 195 nearest void galaxies reside in the Local Volume. We summarize the main statistical properties of the new sample and outline the prospects of study of both, the void dwarf properties and the fine structure of voids.

Keywords

galaxies: dwarfgalaxies: formationgalaxies: evolutiongalaxies: generallarge-scale structure of universecatalogs
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S344: Dwarf Galaxies: From the Deep Universe to the Present , August 2018 , pp. 396 - 399
Copyright
© International Astronomical Union 2019 

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