The isolated interacting galaxy pair NGC 5426/27 (ARP 271)

I. Fuentes-Carrera; M. Rosado; P. Amram; D. Dultzin-Hacyan; A. Bernal; H. Salo; E. Laurikainen; I. Cruz-González; E. Le Coarer

The isolated interacting galaxy pair NGC 5426/27 (ARP 271)

I. Fuentes-Carrera, M. Rosado, P. Amram, D. Dultzin-Hacyan, A. Bernal, H. Salo, E. Laurikainen, I. Cruz-González, E. Le Coarer

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

Abstract

The isolated interacting galaxy pair NGC 5426/27 (Arp 271) was observed using the scanning Fabry-Perot interferometer PUMA. The velocity eld, various kinematical parameters and rotation curve for each galaxy were derived. We found a small bar-like structure in NGC 5426 and a severely distorted velocity field for NGC 5427. A range of possible masses was computed for each galaxy.

Original language	English
Pages (from-to)	134-137
Number of pages	4
Journal	Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias
Volume	10
State	Published - 2001
Externally published	Yes
Event	7th Texas-Mexico Conference on Astrophysics: Flows, Blows and Glows - Austin, TX, United States Duration: 6 Apr 2000 → 8 Apr 2000

Keywords

Galaxies: ISM
Galaxies: individual (NGC 5426, NGC 5427)
Galaxies: interactions
Galaxies: kinematics and dynamics
Galaxies: spiral

Cite this

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title = "The isolated interacting galaxy pair NGC 5426/27 (ARP 271)",

abstract = "The isolated interacting galaxy pair NGC 5426/27 (Arp 271) was observed using the scanning Fabry-Perot interferometer PUMA. The velocity eld, various kinematical parameters and rotation curve for each galaxy were derived. We found a small bar-like structure in NGC 5426 and a severely distorted velocity field for NGC 5427. A range of possible masses was computed for each galaxy.",

keywords = "Galaxies: ISM, Galaxies: individual (NGC 5426, NGC 5427), Galaxies: interactions, Galaxies: kinematics and dynamics, Galaxies: spiral",

author = "I. Fuentes-Carrera and M. Rosado and P. Amram and D. Dultzin-Hacyan and A. Bernal and H. Salo and E. Laurikainen and I. Cruz-Gonz{\'a}lez and {Le Coarer}, E.",

year = "2001",

language = "Ingl{\'e}s",

volume = "10",

pages = "134--137",

journal = "Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias",

issn = "1405-2059",

note = "7th Texas-Mexico Conference on Astrophysics: Flows, Blows and Glows ; Conference date: 06-04-2000 Through 08-04-2000",

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TY - JOUR

T1 - The isolated interacting galaxy pair NGC 5426/27 (ARP 271)

AU - Fuentes-Carrera, I.

AU - Rosado, M.

AU - Amram, P.

AU - Dultzin-Hacyan, D.

AU - Bernal, A.

AU - Salo, H.

AU - Laurikainen, E.

AU - Cruz-González, I.

AU - Le Coarer, E.

PY - 2001

Y1 - 2001

N2 - The isolated interacting galaxy pair NGC 5426/27 (Arp 271) was observed using the scanning Fabry-Perot interferometer PUMA. The velocity eld, various kinematical parameters and rotation curve for each galaxy were derived. We found a small bar-like structure in NGC 5426 and a severely distorted velocity field for NGC 5427. A range of possible masses was computed for each galaxy.

AB - The isolated interacting galaxy pair NGC 5426/27 (Arp 271) was observed using the scanning Fabry-Perot interferometer PUMA. The velocity eld, various kinematical parameters and rotation curve for each galaxy were derived. We found a small bar-like structure in NGC 5426 and a severely distorted velocity field for NGC 5427. A range of possible masses was computed for each galaxy.

KW - Galaxies: ISM

KW - Galaxies: individual (NGC 5426, NGC 5427)

KW - Galaxies: interactions

KW - Galaxies: kinematics and dynamics

KW - Galaxies: spiral

UR - http://www.scopus.com/inward/record.url?scp=70649106319&partnerID=8YFLogxK

M3 - Artículo de la conferencia

AN - SCOPUS:70649106319

SN - 1405-2059

VL - 10

SP - 134

EP - 137

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

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

T2 - 7th Texas-Mexico Conference on Astrophysics: Flows, Blows and Glows

Y2 - 6 April 2000 through 8 April 2000

ER -

The isolated interacting galaxy pair NGC 5426/27 (ARP 271)

Abstract

Keywords

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