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NGC 2748 - A galaxy with a ''failed'' polar ring? / HagenThorn, VA; Reshetnikov, VP; Yakovleva, VA.

In: АСТРОНОМИЧЕСКИЙ ЖУРНАЛ, Vol. 73, No. 1, 1996, p. 36-43.

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

Harvard

HagenThorn, VA, Reshetnikov, VP & Yakovleva, VA 1996, 'NGC 2748 - A galaxy with a ''failed'' polar ring?', АСТРОНОМИЧЕСКИЙ ЖУРНАЛ, vol. 73, no. 1, pp. 36-43.

APA

HagenThorn, VA., Reshetnikov, VP., & Yakovleva, VA. (1996). NGC 2748 - A galaxy with a ''failed'' polar ring? АСТРОНОМИЧЕСКИЙ ЖУРНАЛ, 73(1), 36-43.

Vancouver

HagenThorn VA, Reshetnikov VP, Yakovleva VA. NGC 2748 - A galaxy with a ''failed'' polar ring? АСТРОНОМИЧЕСКИЙ ЖУРНАЛ. 1996;73(1):36-43.

Author

HagenThorn, VA ; Reshetnikov, VP ; Yakovleva, VA. / NGC 2748 - A galaxy with a ''failed'' polar ring?. In: АСТРОНОМИЧЕСКИЙ ЖУРНАЛ. 1996 ; Vol. 73, No. 1. pp. 36-43.

BibTeX

@article{374c7189d0e54040a99edd19a23f6cc5,
title = "NGC 2748 - A galaxy with a ''failed'' polar ring?",
abstract = "Results of photometric (in color bands B, V, and R(c)) and kinematic studies of the peculiar galaxy NGC 2748 are presented. The mass distribution is represented by two-component model consisting of an exponential disk and a spherical halo. It is shown that the main observational features of NGC 2748 - in particular, the presence of diffuse formations extended along the minor axis and the existence of a radial velocity gradient along the minor axis - are most likely a consequence of accretion onto the galaxy of gas from a dwarf satellite.",
keywords = "SPIRAL GALAXIES, STARS",
author = "VA HagenThorn and VP Reshetnikov and VA Yakovleva",
year = "1996",
language = "не определен",
volume = "73",
pages = "36--43",
journal = "АСТРОНОМИЧЕСКИЙ ЖУРНАЛ",
issn = "0004-6299",
publisher = "Международная книга",
number = "1",

}

RIS

TY - JOUR

T1 - NGC 2748 - A galaxy with a ''failed'' polar ring?

AU - HagenThorn, VA

AU - Reshetnikov, VP

AU - Yakovleva, VA

PY - 1996

Y1 - 1996

N2 - Results of photometric (in color bands B, V, and R(c)) and kinematic studies of the peculiar galaxy NGC 2748 are presented. The mass distribution is represented by two-component model consisting of an exponential disk and a spherical halo. It is shown that the main observational features of NGC 2748 - in particular, the presence of diffuse formations extended along the minor axis and the existence of a radial velocity gradient along the minor axis - are most likely a consequence of accretion onto the galaxy of gas from a dwarf satellite.

AB - Results of photometric (in color bands B, V, and R(c)) and kinematic studies of the peculiar galaxy NGC 2748 are presented. The mass distribution is represented by two-component model consisting of an exponential disk and a spherical halo. It is shown that the main observational features of NGC 2748 - in particular, the presence of diffuse formations extended along the minor axis and the existence of a radial velocity gradient along the minor axis - are most likely a consequence of accretion onto the galaxy of gas from a dwarf satellite.

KW - SPIRAL GALAXIES

KW - STARS

M3 - статья

VL - 73

SP - 36

EP - 43

JO - АСТРОНОМИЧЕСКИЙ ЖУРНАЛ

JF - АСТРОНОМИЧЕСКИЙ ЖУРНАЛ

SN - 0004-6299

IS - 1

ER -

ID: 32253755