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Main Authors: Karachentsev, I. D., Popova, A. A.
Format: Preprint
Published: 2024
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Online Access:https://arxiv.org/abs/2407.01287
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author Karachentsev, I. D.
Popova, A. A.
author_facet Karachentsev, I. D.
Popova, A. A.
contents Based on the fluxes of 1400 nearby galaxies observed in far ultraviolet (${\rm FUV}$) and in the H$α$ line, we determined the global star formation rate per unit Universe volume, $j_{\rm SFR}=(1.34\pm0.16) 10^{-2}\,M_{\odot}$ yr$^{-1}$ Mpc$^{-3}$. With the current star formation rate (SFR), ($65\pm4)$% of the observed stellar mass is reproduced in the cosmological time of 13.8 billion years. The neutral gas reserves in the Local Volume with a radius of 11 Mpc will facilitate the current SFR on a scale of approximately another 5 billion years.
format Preprint
id arxiv_https___arxiv_org_abs_2407_01287
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Average Star Formation Parameters in the Local Volume of the Universe
Karachentsev, I. D.
Popova, A. A.
Astrophysics of Galaxies
Based on the fluxes of 1400 nearby galaxies observed in far ultraviolet (${\rm FUV}$) and in the H$α$ line, we determined the global star formation rate per unit Universe volume, $j_{\rm SFR}=(1.34\pm0.16) 10^{-2}\,M_{\odot}$ yr$^{-1}$ Mpc$^{-3}$. With the current star formation rate (SFR), ($65\pm4)$% of the observed stellar mass is reproduced in the cosmological time of 13.8 billion years. The neutral gas reserves in the Local Volume with a radius of 11 Mpc will facilitate the current SFR on a scale of approximately another 5 billion years.
title Average Star Formation Parameters in the Local Volume of the Universe
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2407.01287