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The stellar population study of the polar rings in the galaxies NGC 2685 and NGC 4650A. / Karataeva, G. M.; Drozdovsky, I. O.; Tikhonov, N. A.; Galazutdinova, O. A.; Yakovleva, V. A.

In: Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias, Vol. 17, 01.12.2003.

Research output: Contribution to journal › Conference article › peer-review

Harvard

Karataeva, GM, Drozdovsky, IO, Tikhonov, NA, Galazutdinova, OA & Yakovleva, VA 2003, 'The stellar population study of the polar rings in the galaxies NGC 2685 and NGC 4650A', Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias, vol. 17.

APA

Karataeva, G. M., Drozdovsky, I. O., Tikhonov, N. A., Galazutdinova, O. A., & Yakovleva, V. A. (2003). The stellar population study of the polar rings in the galaxies NGC 2685 and NGC 4650A. Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias, 17.

Vancouver

Karataeva GM, Drozdovsky IO, Tikhonov NA, Galazutdinova OA, Yakovleva VA. The stellar population study of the polar rings in the galaxies NGC 2685 and NGC 4650A. Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias. 2003 Dec 1;17.

Author

Karataeva, G. M. ; Drozdovsky, I. O. ; Tikhonov, N. A. ; Galazutdinova, O. A. ; Yakovleva, V. A. / The stellar population study of the polar rings in the galaxies NGC 2685 and NGC 4650A. In: Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias. 2003 ; Vol. 17.

BibTeX

@article{461a4552d81f49fd8d730e934411920b,
title = "The stellar population study of the polar rings in the galaxies NGC 2685 and NGC 4650A",
abstract = "Polar ring galaxies (PRGs) are dynamically peculiar systems with a ring or annulus of gas, stars and dust orbiting in a plane nearly perpendicular to the equatorial plane of the host galaxy (Withmore 1990). According to the most popular point of view, PRGs are the result of galaxy interaction, which ranges from simple gas accretion to a complete merger. Alternatively, polar rings can represent the delayed inows of primordial gas. Therefore, the problem of PR's age is actual (Eskridge&Podge 1997; Gallagher et al 2002). Deep single-star photometry can directly identify stars in various evolutionary phases through their positions on CMD. This can cast light on the origin and evolution of PRGs.",
author = "Karataeva, {G. M.} and Drozdovsky, {I. O.} and Tikhonov, {N. A.} and Galazutdinova, {O. A.} and Yakovleva, {V. A.}",
year = "2003",
month = dec,
day = "1",
language = "English",
volume = "17",
journal = "Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias",
issn = "1405-2059",
publisher = "Universidad Nacional Autonoma de Mexico",
note = "Galaxy Evolution: Theory and Observations ; Conference date: 08-04-2002 Through 12-04-2002",

}

RIS

TY - JOUR

T1 - The stellar population study of the polar rings in the galaxies NGC 2685 and NGC 4650A

AU - Karataeva, G. M.

AU - Drozdovsky, I. O.

AU - Tikhonov, N. A.

AU - Galazutdinova, O. A.

AU - Yakovleva, V. A.

PY - 2003/12/1

Y1 - 2003/12/1

N2 - Polar ring galaxies (PRGs) are dynamically peculiar systems with a ring or annulus of gas, stars and dust orbiting in a plane nearly perpendicular to the equatorial plane of the host galaxy (Withmore 1990). According to the most popular point of view, PRGs are the result of galaxy interaction, which ranges from simple gas accretion to a complete merger. Alternatively, polar rings can represent the delayed inows of primordial gas. Therefore, the problem of PR's age is actual (Eskridge&Podge 1997; Gallagher et al 2002). Deep single-star photometry can directly identify stars in various evolutionary phases through their positions on CMD. This can cast light on the origin and evolution of PRGs.

AB - Polar ring galaxies (PRGs) are dynamically peculiar systems with a ring or annulus of gas, stars and dust orbiting in a plane nearly perpendicular to the equatorial plane of the host galaxy (Withmore 1990). According to the most popular point of view, PRGs are the result of galaxy interaction, which ranges from simple gas accretion to a complete merger. Alternatively, polar rings can represent the delayed inows of primordial gas. Therefore, the problem of PR's age is actual (Eskridge&Podge 1997; Gallagher et al 2002). Deep single-star photometry can directly identify stars in various evolutionary phases through their positions on CMD. This can cast light on the origin and evolution of PRGs.

UR - http://www.scopus.com/inward/record.url?scp=71949102539&partnerID=8YFLogxK

M3 - Conference article

AN - SCOPUS:71949102539

VL - 17

JO - Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias

JF - Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias

SN - 1405-2059

T2 - Galaxy Evolution: Theory and Observations

Y2 - 8 April 2002 through 12 April 2002

ER -

ID: 40869351