Add to ORKGFrom the photographic photometry of NGC 7764, the integrated apparent magnitude and the morphological parameter qₙ was determined. From the emission lines of the spectrum the radial velocity was estimated in 1729 km/sec. The observed emission spectrum is a typical example of galaxies which show brigth emission regions.Asociación Argentina de Astronomí
The relationships between the Z distance, the Z dispersion and the galactic rotational velocity of n...
En los últimos meses se inició un programa de observación de velocidades radiales de galaxias austra...
Distance and age of NGC 2516 are estimated by UBV photometry. The location of peculiar stars in colo...
From the photographic photometry of NGC 7764, the integrated apparent magnitude and the morphologica...
Las placas del SPM son óptimas para la búsqueda de galaxias puesto que unen a la escala de astrográf...
The object of this work is to classify galaxies with emission lines according to these spectra, so a...
Three-color photoelectric photometry has been carried out for the nuclear regions in NGC 1672 (with ...
Contenido Galaxias Comunicaciones -Un estudio sobre la irregular magallánica NGC 7774 | M. Pa...
Evidence of complex motions in the stellar component of NGC 5128 have been found in several well exp...
This paper presents results which further clarify morphological and thermodynamical aspects of the i...
Spectroscopic and morphological observations suggest that we are dealing with an unstable group of g...
The relative intensities of the hydrogen emission lines of homogeneous gaseous nebulae, ionized and ...
A brief review of radioastronomy fundamentals (types of signals and radiotelescopes) is followed by ...
Tesis (Doctor en Astronomía)--Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y ...
he distribution of light in the Peculiar Galaxy IC 4662 has been studied by means of photographic ph...
The relationships between the Z distance, the Z dispersion and the galactic rotational velocity of n...
En los últimos meses se inició un programa de observación de velocidades radiales de galaxias austra...
Distance and age of NGC 2516 are estimated by UBV photometry. The location of peculiar stars in colo...
From the photographic photometry of NGC 7764, the integrated apparent magnitude and the morphologica...
Las placas del SPM son óptimas para la búsqueda de galaxias puesto que unen a la escala de astrográf...
The object of this work is to classify galaxies with emission lines according to these spectra, so a...
Three-color photoelectric photometry has been carried out for the nuclear regions in NGC 1672 (with ...
Contenido Galaxias Comunicaciones -Un estudio sobre la irregular magallánica NGC 7774 | M. Pa...
Evidence of complex motions in the stellar component of NGC 5128 have been found in several well exp...
This paper presents results which further clarify morphological and thermodynamical aspects of the i...
Spectroscopic and morphological observations suggest that we are dealing with an unstable group of g...
The relative intensities of the hydrogen emission lines of homogeneous gaseous nebulae, ionized and ...
A brief review of radioastronomy fundamentals (types of signals and radiotelescopes) is followed by ...
Tesis (Doctor en Astronomía)--Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y ...
he distribution of light in the Peculiar Galaxy IC 4662 has been studied by means of photographic ph...
The relationships between the Z distance, the Z dispersion and the galactic rotational velocity of n...
En los últimos meses se inició un programa de observación de velocidades radiales de galaxias austra...
Distance and age of NGC 2516 are estimated by UBV photometry. The location of peculiar stars in colo...