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The kinematics of the Wolf-Rayet galaxy pairs NGC 1741 and NGC 7714/7715

Published online by Cambridge University Press:  25 May 2016

Margarita Rosado ,
Leonid Georgiev ,
Deborah Dultzin-Hacyan  and
Irene Cruz-González
Margarita Rosado
Affiliation:
Instituto de Astronomía, UNAM, Apartado Postal 70–264, CP04510, México, D.F., México.
Leonid Georgiev
Affiliation:
Instituto de Astronomía, UNAM, Apartado Postal 70–264, CP04510, México, D.F., México.
Deborah Dultzin-Hacyan
Affiliation:
Instituto de Astronomía, UNAM, Apartado Postal 70–264, CP04510, México, D.F., México.
Irene Cruz-González
Affiliation:
Instituto de Astronomía, UNAM, Apartado Postal 70–264, CP04510, México, D.F., México.

Abstract

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We present preliminary results of the kinematics of the Wolf-Rayet galaxy pairs: NGC 1741 and NGC 7714/7715.

Type
Part 5. Wolf-Rayet stars and other massive stars in starburst galaxies: the case of Wolf-Rayet galaxies (integrated spectra)
Information
Symposium - International Astronomical Union , Volume 193: Wolf-Rayet Phenomena in Massive Stars and Starburst Galaxies , 1999 , pp. 618 - 619
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

González-Delgado, R.M. et al. 1995, ApJ 439, 604 CrossRefGoogle Scholar
Rosado, M. et al. 1995, RevMexAA-SC 3, 263 Google Scholar
Rubin, V.C., Hunter, D.A., Ford, W.K. 1990, ApJ 365, 86 CrossRefGoogle Scholar
Smith, B.J. et al. 1997, ApJ 483, 754 CrossRefGoogle Scholar