We present the burst ages for young stellar populations in a sample of six nearby (<10 Mpc) spiral galaxies using a differential pixel-based analysis of the ionized gas emission. We explore this as an alternative approach for connecting large-scale dynamical mechanisms with star formation processes in disc galaxies, based on burst ages derived from the Hα to far-UV (FUV) flux ratio. Images of each galaxy in Hα were taken with Taurus Tunable Filter and matched to FUV imaging from GALEX. The resulting flux ratio provides a robust measure of relative age across the disc which we discuss in terms of the large-scale dynamical motions. Systematic effects such as a variable initial mass function, non-solar metallicities, variable star formation hi...
We show that the star formation activity of spiral galaxies has a great variety. The star formation ...
The question of how and where galaxies build up their mass over time by converting their gas into st...
We present multiband photometric observations of three spiral galaxies selected in a sample suited f...
We present the burst ages for young stellar populations in a sample of six nearby (< 10 Mpc) spir...
Spiral arms formation is still an open problem. Even in our Galaxy, the number of spiral arms and it...
We map the stellar age distribution (≲1 Gyr) across a 6 kpc × 6 kpc area of the Galactic disc in o...
We explore the radial variation of star formation histories (SFHs) in dwarf galaxies simulated with ...
11 pages, 8 figuresWe study the star formation history of normal spirals by using a large and homoge...
This thesis addresses the stellar population content in the bulges and disks of spiral galaxies usin...
Context. Bright knots along arms are observed in K-band images of many grand-design spiral galaxies....
The bulges of spiral galaxies may be old, as in our Galaxy, or may possess younger stars, as evidenc...
Galaxies in the local Universe are known to follow bimodal distributions in the global stellar popul...
We investigated the properties of the stellar populations in the discs of a sample of 10 spiral gala...
Context. Bright knots along arms are observed in K-band images of many grand-design spiral galaxies....
We present a study of the variation of spatial structure of stellar populations within dwarf galaxie...
We show that the star formation activity of spiral galaxies has a great variety. The star formation ...
The question of how and where galaxies build up their mass over time by converting their gas into st...
We present multiband photometric observations of three spiral galaxies selected in a sample suited f...
We present the burst ages for young stellar populations in a sample of six nearby (< 10 Mpc) spir...
Spiral arms formation is still an open problem. Even in our Galaxy, the number of spiral arms and it...
We map the stellar age distribution (≲1 Gyr) across a 6 kpc × 6 kpc area of the Galactic disc in o...
We explore the radial variation of star formation histories (SFHs) in dwarf galaxies simulated with ...
11 pages, 8 figuresWe study the star formation history of normal spirals by using a large and homoge...
This thesis addresses the stellar population content in the bulges and disks of spiral galaxies usin...
Context. Bright knots along arms are observed in K-band images of many grand-design spiral galaxies....
The bulges of spiral galaxies may be old, as in our Galaxy, or may possess younger stars, as evidenc...
Galaxies in the local Universe are known to follow bimodal distributions in the global stellar popul...
We investigated the properties of the stellar populations in the discs of a sample of 10 spiral gala...
Context. Bright knots along arms are observed in K-band images of many grand-design spiral galaxies....
We present a study of the variation of spatial structure of stellar populations within dwarf galaxie...
We show that the star formation activity of spiral galaxies has a great variety. The star formation ...
The question of how and where galaxies build up their mass over time by converting their gas into st...
We present multiband photometric observations of three spiral galaxies selected in a sample suited f...