Hostname: page-component-7c8c6479df-p566r Total loading time: 0 Render date: 2024-03-28T12:01:19.512Z Has data issue: false hasContentIssue false

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
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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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)
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