Standard

Photometric Study of Two Galaxies with X-Structures. / Reshetnikov, V. P.; Tarakanov, P. A.; Kostina, M. V.

в: Astrophysics, Том 63, № 1, 25.03.2020, стр. 15-22.

Результаты исследований: Научные публикации в периодических изданияхстатьяРецензирование

Harvard

APA

Vancouver

Author

BibTeX

@article{75db64023cd44f5bbbca09f1d1f3f573,
title = "Photometric Study of Two Galaxies with X-Structures",
abstract = "Data from the SDSS survey are used to study two galaxies with X-structures (UGC 501 and UGC 12253) visible from the edge. Both objects are spiral galaxies of late morphological types with extended stellar disks. The X-structures in the galaxies have different sizes and shapes. The possibility that the different observational parameters of the X-structures in UGC 501 and UGC 12253 are related to different characteristics of their underlying galaxies is discussed (primarily in the relative contribution of the dark halo).",
keywords = "galaxies, photometry, morphology, SDSS galaxies, DIGITAL SKY SURVEY, SHAPED STRUCTURES",
author = "Reshetnikov, {V. P.} and Tarakanov, {P. A.} and Kostina, {M. V.}",
note = "Reshetnikov, V.P., Tarakanov, P.A. & Kostina, M.V. Photometric Study of Two Galaxies with X-Structures. Astrophysics (2020). https://doi.org/10.1007/s10511-020-09609-4",
year = "2020",
month = mar,
day = "25",
doi = "https://doi.org/10.1007/s10511-020-09609-4",
language = "English",
volume = "63",
pages = "15--22",
journal = "Astrophysics",
issn = "0571-7256",
publisher = "Wolters Kluwer",
number = "1",

}

RIS

TY - JOUR

T1 - Photometric Study of Two Galaxies with X-Structures

AU - Reshetnikov, V. P.

AU - Tarakanov, P. A.

AU - Kostina, M. V.

N1 - Reshetnikov, V.P., Tarakanov, P.A. & Kostina, M.V. Photometric Study of Two Galaxies with X-Structures. Astrophysics (2020). https://doi.org/10.1007/s10511-020-09609-4

PY - 2020/3/25

Y1 - 2020/3/25

N2 - Data from the SDSS survey are used to study two galaxies with X-structures (UGC 501 and UGC 12253) visible from the edge. Both objects are spiral galaxies of late morphological types with extended stellar disks. The X-structures in the galaxies have different sizes and shapes. The possibility that the different observational parameters of the X-structures in UGC 501 and UGC 12253 are related to different characteristics of their underlying galaxies is discussed (primarily in the relative contribution of the dark halo).

AB - Data from the SDSS survey are used to study two galaxies with X-structures (UGC 501 and UGC 12253) visible from the edge. Both objects are spiral galaxies of late morphological types with extended stellar disks. The X-structures in the galaxies have different sizes and shapes. The possibility that the different observational parameters of the X-structures in UGC 501 and UGC 12253 are related to different characteristics of their underlying galaxies is discussed (primarily in the relative contribution of the dark halo).

KW - galaxies

KW - photometry

KW - morphology

KW - SDSS galaxies

KW - DIGITAL SKY SURVEY

KW - SHAPED STRUCTURES

UR - http://www.scopus.com/inward/record.url?scp=85082968060&partnerID=8YFLogxK

UR - https://www.mendeley.com/catalogue/73982546-c296-3fb6-981f-8f0a0096743c/

U2 - https://doi.org/10.1007/s10511-020-09609-4

DO - https://doi.org/10.1007/s10511-020-09609-4

M3 - Article

AN - SCOPUS:85082968060

VL - 63

SP - 15

EP - 22

JO - Astrophysics

JF - Astrophysics

SN - 0571-7256

IS - 1

ER -

ID: 52509338