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 -