Add to ORKGSpectro-photometric observations of 63 stars of the Orion aggregate have been made. Relative energy distributions and equivalent widths of Hβ, Hγ and Hδ have been measured. The results will be used for a relative magnitude calibration.Asociación Argentina de Astronomí
Han sido analizados 20 espectros tomados en Córdoba, Sudáfrica y Cerro Tololo, estudiándose las medi...
De 42 perfiles de la Imea de 21 cm., se dedujo la distribución del hidrógeno neutro en la región de ...
We studied the 21 cm line of the interstellar neutral hydrogen of three dark regions catalogued by F...
Spectro-photometric observations of 63 stars of the Orion aggregate have been made. Relative energy ...
Three color photoelectric photometry is presented for 43 stars in the vicinity of the southern galac...
The spectra of some thirty Be stars are described, based upon spectrograms obtained at Flagstaff and...
Presentamos fotometría CCD UBVIKC para los cúmulos abiertos (CAs) NGC 2311, Trumpler 6, NGC 2432 y B...
We report on both high-precision photometry from the Microvariability and Oscillations of Stars (MOS...
Tesis doctoral inédita leída en la Universidad Autónoma de Madrid, Facultad de Ciencias, Departament...
We present the first results of the Accretion Discs in Hα with OmegaCAM (ADHOC) survey, which aims t...
Galaxies are the building blocks of the Universe. Understanding their role in the cosmos translates ...
We present U, B, V, I broadband, 6200 Å TiO mediumband, and Hα narrowband photometry of the Orion Ne...
A photoelectric spectrum scanner attached to the 16-inch telescope of the Cerro Tololo Inter-America...
Aims. We study in detail nine sources in the direction of the young σ Orionis cluster, which is cons...
From the photographic photometry of NGC 7764, the integrated apparent magnitude and the morphologica...
Han sido analizados 20 espectros tomados en Córdoba, Sudáfrica y Cerro Tololo, estudiándose las medi...
De 42 perfiles de la Imea de 21 cm., se dedujo la distribución del hidrógeno neutro en la región de ...
We studied the 21 cm line of the interstellar neutral hydrogen of three dark regions catalogued by F...
Spectro-photometric observations of 63 stars of the Orion aggregate have been made. Relative energy ...
Three color photoelectric photometry is presented for 43 stars in the vicinity of the southern galac...
The spectra of some thirty Be stars are described, based upon spectrograms obtained at Flagstaff and...
Presentamos fotometría CCD UBVIKC para los cúmulos abiertos (CAs) NGC 2311, Trumpler 6, NGC 2432 y B...
We report on both high-precision photometry from the Microvariability and Oscillations of Stars (MOS...
Tesis doctoral inédita leída en la Universidad Autónoma de Madrid, Facultad de Ciencias, Departament...
We present the first results of the Accretion Discs in Hα with OmegaCAM (ADHOC) survey, which aims t...
Galaxies are the building blocks of the Universe. Understanding their role in the cosmos translates ...
We present U, B, V, I broadband, 6200 Å TiO mediumband, and Hα narrowband photometry of the Orion Ne...
A photoelectric spectrum scanner attached to the 16-inch telescope of the Cerro Tololo Inter-America...
Aims. We study in detail nine sources in the direction of the young σ Orionis cluster, which is cons...
From the photographic photometry of NGC 7764, the integrated apparent magnitude and the morphologica...
Han sido analizados 20 espectros tomados en Córdoba, Sudáfrica y Cerro Tololo, estudiándose las medi...
De 42 perfiles de la Imea de 21 cm., se dedujo la distribución del hidrógeno neutro en la región de ...
We studied the 21 cm line of the interstellar neutral hydrogen of three dark regions catalogued by F...