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Peculiarities in the formation of molecular clouds in the central regions of spiral galaxies. / Volkov, E. V.

в: Astrophysics, Том 47, № 3, 07.2004, стр. 335-342.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

Harvard

Volkov, EV 2004, 'Peculiarities in the formation of molecular clouds in the central regions of spiral galaxies', Astrophysics, Том. 47, № 3, стр. 335-342. https://doi.org/10.1023/B:ASYS.0000040162.33710.bc

APA

Volkov, E. V. (2004). Peculiarities in the formation of molecular clouds in the central regions of spiral galaxies. Astrophysics, 47(3), 335-342. https://doi.org/10.1023/B:ASYS.0000040162.33710.bc

Vancouver

Volkov EV. Peculiarities in the formation of molecular clouds in the central regions of spiral galaxies. Astrophysics. 2004 Июль;47(3):335-342. https://doi.org/10.1023/B:ASYS.0000040162.33710.bc

Author

Volkov, E. V. / Peculiarities in the formation of molecular clouds in the central regions of spiral galaxies. в: Astrophysics. 2004 ; Том 47, № 3. стр. 335-342.

BibTeX

@article{467b8527e3264ac99d8d78c10fd336d8,
title = "Peculiarities in the formation of molecular clouds in the central regions of spiral galaxies",
abstract = "The limitations imposed by the shear instability on the formation of gigantic molecular clouds in the central regions of spiral galaxies are examined. The criteria obtained here are illustrated using the example of six galaxies for which the detailed rotation curves are known. The different mechanisms for formation of molecular clouds which apply in the central and edge regions of disk galaxies are evaluated.",
keywords = "molecular clouds, shear instability",
author = "Volkov, {E. V.}",
note = "Copyright: Copyright 2012 Elsevier B.V., All rights reserved.",
year = "2004",
month = jul,
doi = "10.1023/B:ASYS.0000040162.33710.bc",
language = "English",
volume = "47",
pages = "335--342",
journal = "Astrophysics",
issn = "0571-7256",
publisher = "Wolters Kluwer",
number = "3",

}

RIS

TY - JOUR

T1 - Peculiarities in the formation of molecular clouds in the central regions of spiral galaxies

AU - Volkov, E. V.

N1 - Copyright: Copyright 2012 Elsevier B.V., All rights reserved.

PY - 2004/7

Y1 - 2004/7

N2 - The limitations imposed by the shear instability on the formation of gigantic molecular clouds in the central regions of spiral galaxies are examined. The criteria obtained here are illustrated using the example of six galaxies for which the detailed rotation curves are known. The different mechanisms for formation of molecular clouds which apply in the central and edge regions of disk galaxies are evaluated.

AB - The limitations imposed by the shear instability on the formation of gigantic molecular clouds in the central regions of spiral galaxies are examined. The criteria obtained here are illustrated using the example of six galaxies for which the detailed rotation curves are known. The different mechanisms for formation of molecular clouds which apply in the central and edge regions of disk galaxies are evaluated.

KW - molecular clouds

KW - shear instability

UR - http://www.scopus.com/inward/record.url?scp=4544303220&partnerID=8YFLogxK

U2 - 10.1023/B:ASYS.0000040162.33710.bc

DO - 10.1023/B:ASYS.0000040162.33710.bc

M3 - Article

AN - SCOPUS:4544303220

VL - 47

SP - 335

EP - 342

JO - Astrophysics

JF - Astrophysics

SN - 0571-7256

IS - 3

ER -

ID: 77691474