1. |
Very high energy cosmic gamma radiation : a crucial window on the extreme universe.
|
2004 |
Libro |
143.007 AHA
|
2. |
JENAM 2002 : galactic & stellar dynamics / edited by C. M. Boily, O. Patsis, S. Portegies Zwart, R. Spurzem and C. Theis.
|
2003 |
Libro |
160 BOI
|
3. |
A radio continuum and HI line study of the Perseus cluster.
|
1993 |
Tesis |
016.146
|
4. |
Efectos de alineamientos en galaxias y cúmulos de galaxias / Hernán Muriel; director Diego García Lambas.
|
1992 |
Tesis |
016 MUR
|
5. |
The structure of rich clusters of galaxies: clues to formation and origen.
|
1989 |
Tesis |
016.139
|
6. |
The Minnesota lectures on clusters of galaxies and large-scale structure.
|
1988 |
Libro |
160.005
|
7. |
Observational cosmology : proceedings of the 124th Symposium of the International Astronomical Union, held in Beijing, China, August 25-30, 1986 / edited by Adelaide Hewitt, Geoffrey Burbidge, and Li Zhi Fang.
|
1987 |
Libro |
006.111
|
8. |
HI properties of spiral galaxies in the virgo cluster.
|
1986 |
Tesis |
016.148
|
9. |
Structure and evolution of the Magellanic Clouds / edited by Sidney van den Bergh and Klaas S. de Boer.
|
1984 |
Libro |
006.095
|
10. |
Groups and clusters of galaxies : radio and x-ray studies.
|
1984 |
Tesis |
016.084
|
11. |
Clustering in the universe.
|
1983 |
Libro |
160.003
|
12. |
Radio emission in the Virgo cluster and in SO galaxies.
|
1981 |
Tesis |
016.085
|
13. |
Extragalactic high energy astrophysics.
|
1979 |
Libro |
160.004
|
14. |
Radio investigations of clusters of galaxies : a study of radio luminosity functions, wide-angle head-tailed radio galaxies and cluster radio haloes with the Westerbork Synthesis Radio Telescope.
|
1978 |
Tesis |
016.016
|
15. |
Hidrógeno neutro en cúmulos galácticos.
|
1977 |
Libro |
016.011
|
16. |
Radio galaxies and the intergalactic material in clusters.
|
1974 |
Tesis |
016.068
|
17. |
Formation of galaxies inside clusters.
|
1972 |
Tesis |
016.065
|
18. |
Galaxy clustering : its description and its interpretacion.
|
1969 |
Libro |
160.001
|