Add to ORKGHα images of 20 nearby Southern galaxies were obtained using narrow interferometric filters. Positions, fluxes and diameters of the objects were obtained from these frames. A study of the completeness of the sample is made and after a proper calibration, the absolute fluxes and the Hα luminosity function were obtained for each galaxy. Two galaxies in the sample (NGC 1672, NGC 5861) show profiles of type II luminosity function while NGC 6221 shows extended Hα emission.Asociación Argentina de Astronomí
We analyze the statistical properties of the circumnuclear H II regions of a sample of 52 nearby gal...
LaTex, 24 pages, 12 figuresWe have collected a large body of NIR (H band), UV (2000 A) and Halpha me...
The H II region luminosity function (LF) is an important tool for deriving the birthrates and mass d...
By means of CCD frames and image processing techniques we measured the luminosity function of H-alph...
We constructed a local luminosity function (LF) of galaxies using a flux-limited sample (S_170 > 0.1...
We present the first study of GALEX far ultra-violet (FUV) luminosity functions of individual star-f...
The Universidad Complutense de Madrid (UCM) survey is a long-term project aimed at finding and analy...
We use narrow-band imaging (full width at half-maximum = 70 Å) to select a sample of emission-line g...
Context. Statistical properties of HII region populations in disk galaxies yield important clues to ...
We use an unprecedented sample of about 23 000 H II regions detected at an average physical resoluti...
We determined the relative spatial density of the Coma Cluster galaxies, selected by luminosity and ...
To investigate the correlation between optical luminosity and Hi mass, we obtained 21cm Hi line obse...
International audienceWe use an unprecedented sample of about 23 000 H II regions detected at an ave...
The star formation rate (SFR) is one of the main parameters used to analyze the evolution of galaxie...
The galaxy luminosity function describes the number of galaxies per unit volume per unit luminosity....
We analyze the statistical properties of the circumnuclear H II regions of a sample of 52 nearby gal...
LaTex, 24 pages, 12 figuresWe have collected a large body of NIR (H band), UV (2000 A) and Halpha me...
The H II region luminosity function (LF) is an important tool for deriving the birthrates and mass d...
By means of CCD frames and image processing techniques we measured the luminosity function of H-alph...
We constructed a local luminosity function (LF) of galaxies using a flux-limited sample (S_170 > 0.1...
We present the first study of GALEX far ultra-violet (FUV) luminosity functions of individual star-f...
The Universidad Complutense de Madrid (UCM) survey is a long-term project aimed at finding and analy...
We use narrow-band imaging (full width at half-maximum = 70 Å) to select a sample of emission-line g...
Context. Statistical properties of HII region populations in disk galaxies yield important clues to ...
We use an unprecedented sample of about 23 000 H II regions detected at an average physical resoluti...
We determined the relative spatial density of the Coma Cluster galaxies, selected by luminosity and ...
To investigate the correlation between optical luminosity and Hi mass, we obtained 21cm Hi line obse...
International audienceWe use an unprecedented sample of about 23 000 H II regions detected at an ave...
The star formation rate (SFR) is one of the main parameters used to analyze the evolution of galaxie...
The galaxy luminosity function describes the number of galaxies per unit volume per unit luminosity....
We analyze the statistical properties of the circumnuclear H II regions of a sample of 52 nearby gal...
LaTex, 24 pages, 12 figuresWe have collected a large body of NIR (H band), UV (2000 A) and Halpha me...
The H II region luminosity function (LF) is an important tool for deriving the birthrates and mass d...