Astronomy and Astrophysics – Astrophysics
Scientific paper
Mar 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001rmxac..10..134f&link_type=abstract
The Seventh Texas-Mexico Conference on Astrophysics: Flows, Blows and Glows (Eds. William H. Lee and Silvia Torres-Peimbert) Rev
Astronomy and Astrophysics
Astrophysics
Galaxies: Individual (Ngc 5426, Ngc 5427), Galaxies: Interactions, Galaxies: Ism, Galaxies: Kinematics And Dynamics, Galaxies: Spiral
Scientific paper
The isolated interacting galaxy pair NGC 5426/27 (Arp 271) was observed using the scanning Fabry-Perot interferometer PUMA. The velocity field, 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.
Amram Ph.
Bernal Argelia
Cruz-Gonzalez Irene
Dultzin-Hacyan Deborah
Fuentes-Carrera Isaura
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