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Autor Rego Fernández, Manuel |
Documentos disponibles escritos por este autor (26)
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Gallego Maestro, Jesús ; Zamorano Calvo, Jaime ; Rego Fernández, Manuel ; Vitores, A.G. | Kluwer Academic Publ. | 1996The Universidad Complutense de Madrid survey is a long-term project with the aim of finding and analyzing star forming galaxies using the H? line as the tracer for star formation processes. In order to obtain a representative and complete sample[...]texto impreso
Zamorano Calvo, Jaime ; Gallego Maestro, Jesús ; Rego Fernández, Manuel ; Vitores, A. G. ; Alonso, O. | University Chicago Press | 1996-08A low-dispersion objective-prism survey for low-redshift emission-line galaxies (ELGs) is being carried out by the Universidad Complutense de Madrid with the Schmidt telescope at the German-Spanish Observatory of Calar Alto (Almeria, Spain). A 4[...]texto impreso
Alonso, O. ; García Dabó, C. E. ; Zamorano Calvo, Jaime ; Gallego Maestro, Jesús ; Rego Fernández, Manuel | University Chicago Press | 1999-06A new low-dispersion objective-prism search for low-redshift (ztexto impreso
Zamorano Calvo, Jaime ; Rego Fernández, Manuel ; Gallego Maestro, Jesús ; Vitores, A. G. ; González Riestra, R. ; Rodríguez Caderot, Gracia | University Chicago Press | 1994-12A low-dispersion objective-prism survey for low-redshift emission-line galaxies (ELGs) is being carried out by the University Complutense de Madrid with the Schmidt telescope at the German-Spanish Observatory of Calar Alto (Almeria, Spain). A 4°[...]texto impreso
Gallego Maestro, Jesús ; Zamorano Calvo, Jaime ; Aragón Salamanca, A. ; Rego Fernández, Manuel | American Astronomical Society | 1995-12-10The Universidad Complutense de Madrid (UCM) survey is a long-term project aimed at finding and analyzing star-forming galaxies detected by their H? emission in Schmidt objective-prism plates. The instrumental setup limits the volume of the unive[...]texto impreso
Gallego Maestro, Jesús ; García Dabó, C. E. ; Zamorano Calvo, Jaime ; Aragón Salamanca, A. ; Rego Fernández, Manuel | American Astronomical Society | 2002-05-01The measurement of the star formation rate density of the universe is of prime importance in understanding the formation and evolution of galaxies. The [O II] ?3727 emission-line flux, easy to measure up to z ? 1.4 within deep redshift surveys i[...]texto impreso
Gallego Maestro, Jesús ; García Dabó, C. E. ; Zamorano Calvo, Jaime ; Aragón Salamanca, A. ; Rego Fernández, Manuel | Univ. Chicago Press | 2002-05-01The measurement of the star formation rate density of the universe is of prime importance in understanding the formation and evolution of galaxies. The [O ii] ?3727 emission-line flux, easy to measure up to z ? 1.4 within deep redshift surveys i[...]texto impreso
Rego Fernández, Manuel ; González Riestra, R. ; Fernández Figueroa, María José | EDP Sciencies | 1983The ? 1640 feature has been observed in a sample of late type stars of different luminosity classes. The intensity was measured from IUE low dispersion spectra, and it has been compared with the observed X-ray fluxes, finding a relationship bet[...]texto impreso
Fernández Figueroa, María José ; Castro Rubio, Elisa de ; Rego Fernández, Manuel | EDP Sciencies | 1981Observations of ? Ceti (HD 20630), G5 V, obtained with the IUE satellite have been analysed to determine the structure of its outer atmosphere. This analysis is used to derive a model of transition region and to examine the terms of energy balan[...]texto impreso
Zamorano Calvo, Jaime ; Gallego Maestro, Jesús ; Rego Fernández, Manuel ; Vitores, A. G. ; González Riestra, R. | IOP publishing ltd | 1992-09Multiwavelength observations of the galaxy UCM 2257+2438 found in the Universidad Complutense of Madrid (UCM) objective-prism survey are reported. The optic spectroscopy, CCD imaging, near-infrared and IRAS photometric data suggest that this obj[...]texto impreso
Rego Fernández, Manuel ; Cordero Gracia, M. ; Gallego Maestro, Jesús ; Zamorano Calvo, Jaime | EDP Sciencies | 1998-02UCM1612+1308 is a new emission-line galaxy identified in the context of the Universidad Complutense de Madrid (UCM) survey. This object was classified as Blue Compact Galaxy (BCG) from photometric data. A detailed spectroscopic study from new op[...]