Eleven Local Volume dwarf galaxies in the FASHI survey

Fuente: arXiv
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Main Authors: Nazarova, Aleksandra, Makarov, Dmitry, Karachentsev, Igor, Zhang, Chuan-Peng, Zhu, Ming
Format: Preprint
Published: 2025
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author Nazarova, Aleksandra
Makarov, Dmitry
Karachentsev, Igor
Zhang, Chuan-Peng
Zhu, Ming
author_facet Nazarova, Aleksandra
Makarov, Dmitry
Karachentsev, Igor
Zhang, Chuan-Peng
Zhu, Ming
contents We determined HI parameters for eleven nearby late-type dwarf galaxies using FASHI data cubes, despite the fact that the first version of the FASHI catalog does not list any radio sources that could correspond to these galaxies. Four of them are probable peripheral satellites of the bright spiral galaxies: NGC 3556, NGC 4258, NGC 4274, NGC 4490, while others are isolated objects. The considered sample has the following median parameters: a heliocentric velocity of $V_\mathrm{h} = 542 \ km/s$, an HI-line width of $W_\mathrm{50} = 28 \ km/s$, an hydrogen mass of $\log (M_{HI} / M_\odot) = 6.83$, a stellar mass of $\log (M_\star / M_\odot) = 7.19$, and a specific star formation rate of $\mathrm{sSFR} = -10.17 \ yr^{-1}$.
format Preprint
id arxiv_https___arxiv_org_abs_2509_12828
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Eleven Local Volume dwarf galaxies in the FASHI survey
Nazarova, Aleksandra
Makarov, Dmitry
Karachentsev, Igor
Zhang, Chuan-Peng
Zhu, Ming
Astrophysics of Galaxies
We determined HI parameters for eleven nearby late-type dwarf galaxies using FASHI data cubes, despite the fact that the first version of the FASHI catalog does not list any radio sources that could correspond to these galaxies. Four of them are probable peripheral satellites of the bright spiral galaxies: NGC 3556, NGC 4258, NGC 4274, NGC 4490, while others are isolated objects. The considered sample has the following median parameters: a heliocentric velocity of $V_\mathrm{h} = 542 \ km/s$, an HI-line width of $W_\mathrm{50} = 28 \ km/s$, an hydrogen mass of $\log (M_{HI} / M_\odot) = 6.83$, a stellar mass of $\log (M_\star / M_\odot) = 7.19$, and a specific star formation rate of $\mathrm{sSFR} = -10.17 \ yr^{-1}$.
title Eleven Local Volume dwarf galaxies in the FASHI survey
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2509.12828