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On the statistics of galactic warps. / Reshetnikov, V.P.

In: Astronomical and Astrophysical Transactions. Journal of the Eurasian Astronomical Society, Vol. 8, No. 1, 1995, p. 31-37.

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Harvard

Reshetnikov, VP 1995, 'On the statistics of galactic warps', Astronomical and Astrophysical Transactions. Journal of the Eurasian Astronomical Society, vol. 8, no. 1, pp. 31-37. https://doi.org/10.1080/10556799508203294

APA

Reshetnikov, V. P. (1995). On the statistics of galactic warps. Astronomical and Astrophysical Transactions. Journal of the Eurasian Astronomical Society, 8(1), 31-37. https://doi.org/10.1080/10556799508203294

Vancouver

Reshetnikov VP. On the statistics of galactic warps. Astronomical and Astrophysical Transactions. Journal of the Eurasian Astronomical Society. 1995;8(1):31-37. https://doi.org/10.1080/10556799508203294

Author

Reshetnikov, V.P. / On the statistics of galactic warps. In: Astronomical and Astrophysical Transactions. Journal of the Eurasian Astronomical Society. 1995 ; Vol. 8, No. 1. pp. 31-37.

BibTeX

@article{6690ecc1f7784affb993ef7ab0f751f4,
title = "On the statistics of galactic warps",
abstract = "A complete sample of 120 northern galaxies of angular diameters a > 2 arcmin and apparent axial ratio a/b > 7 (Karachentsev et al., 1992) is considered. It is found that at least 50-60% of spiral galaxies exhibit warps in outer parts of optical disks with typical amplitude 4°-5°. The observed frequency of warped galaxies does not show significant dependence on morphological type: spirals of all types demonstrate warped disks. Disks of more massive, large and luminous galaxies are, probably, somewhat less warped.",
keywords = "galaxies, warps",
author = "V.P. Reshetnikov",
year = "1995",
doi = "10.1080/10556799508203294",
language = "English",
volume = "8",
pages = "31--37",
journal = "Astronomical and Astrophysical Transactions",
issn = "1055-6796",
publisher = "Cambridge Scientific Publishers",
number = "1",

}

RIS

TY - JOUR

T1 - On the statistics of galactic warps

AU - Reshetnikov, V.P.

PY - 1995

Y1 - 1995

N2 - A complete sample of 120 northern galaxies of angular diameters a > 2 arcmin and apparent axial ratio a/b > 7 (Karachentsev et al., 1992) is considered. It is found that at least 50-60% of spiral galaxies exhibit warps in outer parts of optical disks with typical amplitude 4°-5°. The observed frequency of warped galaxies does not show significant dependence on morphological type: spirals of all types demonstrate warped disks. Disks of more massive, large and luminous galaxies are, probably, somewhat less warped.

AB - A complete sample of 120 northern galaxies of angular diameters a > 2 arcmin and apparent axial ratio a/b > 7 (Karachentsev et al., 1992) is considered. It is found that at least 50-60% of spiral galaxies exhibit warps in outer parts of optical disks with typical amplitude 4°-5°. The observed frequency of warped galaxies does not show significant dependence on morphological type: spirals of all types demonstrate warped disks. Disks of more massive, large and luminous galaxies are, probably, somewhat less warped.

KW - galaxies

KW - warps

U2 - 10.1080/10556799508203294

DO - 10.1080/10556799508203294

M3 - Article

VL - 8

SP - 31

EP - 37

JO - Astronomical and Astrophysical Transactions

JF - Astronomical and Astrophysical Transactions

SN - 1055-6796

IS - 1

ER -

ID: 5419899