Standard

Specific properties of the aggregation process in the system of molecular clouds in spiral galaxies. / Sotnikova, N. Ya; Volkov, E. V.

In: Astronomy Letters, Vol. 22, No. 5, 01.09.1996, p. 697-702.

Research output: Contribution to journal › Article › peer-review

Harvard

Sotnikova, NY & Volkov, EV 1996, 'Specific properties of the aggregation process in the system of molecular clouds in spiral galaxies', Astronomy Letters, vol. 22, no. 5, pp. 697-702.

APA

Sotnikova, N. Y., & Volkov, E. V. (1996). Specific properties of the aggregation process in the system of molecular clouds in spiral galaxies. Astronomy Letters, 22(5), 697-702.

Vancouver

Sotnikova NY, Volkov EV. Specific properties of the aggregation process in the system of molecular clouds in spiral galaxies. Astronomy Letters. 1996 Sep 1;22(5):697-702.

Author

Sotnikova, N. Ya ; Volkov, E. V. / Specific properties of the aggregation process in the system of molecular clouds in spiral galaxies. In: Astronomy Letters. 1996 ; Vol. 22, No. 5. pp. 697-702.

BibTeX

@article{07afb8238bd04c51b7995c5da7c7c1c2,
title = "Specific properties of the aggregation process in the system of molecular clouds in spiral galaxies",
abstract = "Results of numerical modeling of the evolution of an ensemble of giant molecular clouds in a spiral galaxy are presented. These results are used to demonstrate limitations of the formalism based on the Smoluchowski equation, which is commonly employed in various problems of aggregation. The mass spectra of the clouds obtained from direct modeling are flatter than the spectrum corresponding to the solution of the Smoluchowski equation. The reasons for this difference in the spectra are discussed.",
author = "Sotnikova, {N. Ya} and Volkov, {E. V.}",
year = "1996",
month = sep,
day = "1",
language = "English",
volume = "22",
pages = "697--702",
journal = "Astronomy Letters",
issn = "1063-7737",
publisher = "МАИК {"}Наука/Интерпериодика{"}",
number = "5",

}

RIS

TY - JOUR

T1 - Specific properties of the aggregation process in the system of molecular clouds in spiral galaxies

AU - Sotnikova, N. Ya

AU - Volkov, E. V.

PY - 1996/9/1

Y1 - 1996/9/1

N2 - Results of numerical modeling of the evolution of an ensemble of giant molecular clouds in a spiral galaxy are presented. These results are used to demonstrate limitations of the formalism based on the Smoluchowski equation, which is commonly employed in various problems of aggregation. The mass spectra of the clouds obtained from direct modeling are flatter than the spectrum corresponding to the solution of the Smoluchowski equation. The reasons for this difference in the spectra are discussed.

AB - Results of numerical modeling of the evolution of an ensemble of giant molecular clouds in a spiral galaxy are presented. These results are used to demonstrate limitations of the formalism based on the Smoluchowski equation, which is commonly employed in various problems of aggregation. The mass spectra of the clouds obtained from direct modeling are flatter than the spectrum corresponding to the solution of the Smoluchowski equation. The reasons for this difference in the spectra are discussed.

UR - http://www.scopus.com/inward/record.url?scp=0030493957&partnerID=8YFLogxK

M3 - Article

AN - SCOPUS:0030493957

VL - 22

SP - 697

EP - 702

JO - Astronomy Letters

JF - Astronomy Letters

SN - 1063-7737

IS - 5

ER -

ID: 35162682