Modification to the Jeans criterion by external tides: anisotropic fragmentation and formation of filaments

ABSTRACT The Jeans criterion sets the foundation of our understanding of gravitational collapse. Jog studied the fragmentation of gas under external tides and derived a dispersion relation $l^{\prime } = l_{\rm Jeans} \frac{1}{(1 + \lambda _0^{\prime } / 4 \pi G \rho _0)^{1/2}} \,\,.$ She further co...

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Published inMonthly notices of the Royal Astronomical Society Vol. 532; no. 1; pp. 1126 - 1128
Main Author Li, Guang-Xing
Format Journal Article
LanguageEnglish
Published London Oxford University Press 01.07.2024
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ISSN0035-8711
1365-2966
DOI10.1093/mnras/stae900

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Abstract ABSTRACT The Jeans criterion sets the foundation of our understanding of gravitational collapse. Jog studied the fragmentation of gas under external tides and derived a dispersion relation $l^{\prime } = l_{\rm Jeans} \frac{1}{(1 + \lambda _0^{\prime } / 4 \pi G \rho _0)^{1/2}} \,\,.$ She further concludes that the Jeans mass is $m_{\rm incorrect}^{\prime }=m_{\rm Jeans} [1/(1 + \lambda _0^{\prime } / 4 \pi G \rho _0)^{3/2}]$. We clarify that due to the inhomogeneous nature of tides, this characteristic mass is incorrect. Under weak tides, the mass is $m \approx \rho \, l_1 l_2 l_3$, where the modifications to Jeans lengths along all three dimensions need to be considered; when the tide is strong enough, collapse can only occur once 1 or 2 dimensions. In the latter case, tides can stretch the gas, leading to the formation of filaments.
AbstractList The Jeans criterion sets the foundation of our understanding of gravitational collapse. Jog studied the fragmentation of gas under external tides and derived a dispersion relation $l^{\prime } = l_{\rm Jeans} \frac{1}{(1 + \lambda _0^{\prime } / 4 \pi G \rho _0)^{1/2}} \,\,.$ She further concludes that the Jeans mass is $m_{\rm incorrect}^{\prime }=m_{\rm Jeans} [1/(1 + \lambda _0^{\prime } / 4 \pi G \rho _0)^{3/2}]$. We clarify that due to the inhomogeneous nature of tides, this characteristic mass is incorrect. Under weak tides, the mass is $m \approx \rho \, l_1 l_2 l_3$, where the modifications to Jeans lengths along all three dimensions need to be considered; when the tide is strong enough, collapse can only occur once 1 or 2 dimensions. In the latter case, tides can stretch the gas, leading to the formation of filaments.
ABSTRACT The Jeans criterion sets the foundation of our understanding of gravitational collapse. Jog studied the fragmentation of gas under external tides and derived a dispersion relation $l^{\prime } = l_{\rm Jeans} \frac{1}{(1 + \lambda _0^{\prime } / 4 \pi G \rho _0)^{1/2}} \,\,.$ She further concludes that the Jeans mass is $m_{\rm incorrect}^{\prime }=m_{\rm Jeans} [1/(1 + \lambda _0^{\prime } / 4 \pi G \rho _0)^{3/2}]$. We clarify that due to the inhomogeneous nature of tides, this characteristic mass is incorrect. Under weak tides, the mass is $m \approx \rho \, l_1 l_2 l_3$, where the modifications to Jeans lengths along all three dimensions need to be considered; when the tide is strong enough, collapse can only occur once 1 or 2 dimensions. In the latter case, tides can stretch the gas, leading to the formation of filaments.
Author Li, Guang-Xing
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Cites_doi 10.1093/mnrasl/slt077
10.1093/mnrasl/slad149
10.1093/mnras/stad2091
10.1086/157156
10.1098/rsta.1902.0012
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Issue 1
Keywords methods: analytical
ISM: clouds
galaxies: star formation
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Jeans (2024070322074036000_bib1) 1902; 199
Jog (2024070322074036000_bib2) 2013; 434
Li (2024070322074036000_bib3) 2024; 528
White (2024070322074036000_bib4) 1979; 231
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Snippet ABSTRACT The Jeans criterion sets the foundation of our understanding of gravitational collapse. Jog studied the fragmentation of gas under external tides and...
The Jeans criterion sets the foundation of our understanding of gravitational collapse. Jog studied the fragmentation of gas under external tides and derived a...
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SubjectTerms Criteria
Filaments
Fragmentation
Gravitational collapse
Tides
Title Modification to the Jeans criterion by external tides: anisotropic fragmentation and formation of filaments
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