This paper explores the quantitative connection between globular clusters and the 'diffuse' stellar population of the galaxies they are associated with. Both NGC 1399 and NGC 4486 (M87) are well suited for this kind of analysis due to their large globular cluster populations. The main assumption of our Monte Carlo based models is that each globular cluster is formed along with a given diffuse stellar mass that shares the same spatial distribution, chemical composition and age. The main globular cluster subpopulations, that determine the observed bimodal colour distribution, are decomposed avoiding a priori parametric (e.g. Gaussian) fits and using a new colour (C - T 1)-metallicity relation. The eventual detectability of a 'blue' tilt in th...
A large number of early-type galaxies are now known to possess blue and red subpopulations of globul...
Original paper can be found at: http://www.astrosociety.org/pubs/cs/286.html--Copyright Astronomical...
We present Gemini griz' photometry for 521 globular cluster (GC) candidates in a 5.5 × 5.5 arcmin2 f...
This paper explores the quantitative connection between globular clusters and the 'diffuse' stellar ...
This paper explores the quantitative connection between globular clusters and the 'diffuse' stellar ...
This paper explores the quantitative connection between globular clusters and the “diffuse” stellar ...
As shown in previous works, globular clusters (GCs) can be used to trace the overall structure of th...
As shown in previous works, globular clusters (GCs) can be used to trace the overall structure of th...
This paper explores if, and to what an extent, the stellar populations of early-type galaxies can be...
Globular cluster systems (GCSs) frequently show a bimodal distribution of cluster integrated colours...
This paper explores if, and to what an extent, the stellar populations of early-type galaxies can be...
Globular cluster systems (GCSs) frequently show a bimodal distribution of cluster integrated colours...
Globular cluster systems (GCSs) frequently show a bimodal distribution of cluster integrated colours...
Globular cluster systems (GCS) frequently show a bi-modal distribution of the cluster integrated col...
A large number of early-type galaxies are now known to possess blue and red subpopulations of globul...
A large number of early-type galaxies are now known to possess blue and red subpopulations of globul...
Original paper can be found at: http://www.astrosociety.org/pubs/cs/286.html--Copyright Astronomical...
We present Gemini griz' photometry for 521 globular cluster (GC) candidates in a 5.5 × 5.5 arcmin2 f...
This paper explores the quantitative connection between globular clusters and the 'diffuse' stellar ...
This paper explores the quantitative connection between globular clusters and the 'diffuse' stellar ...
This paper explores the quantitative connection between globular clusters and the “diffuse” stellar ...
As shown in previous works, globular clusters (GCs) can be used to trace the overall structure of th...
As shown in previous works, globular clusters (GCs) can be used to trace the overall structure of th...
This paper explores if, and to what an extent, the stellar populations of early-type galaxies can be...
Globular cluster systems (GCSs) frequently show a bimodal distribution of cluster integrated colours...
This paper explores if, and to what an extent, the stellar populations of early-type galaxies can be...
Globular cluster systems (GCSs) frequently show a bimodal distribution of cluster integrated colours...
Globular cluster systems (GCSs) frequently show a bimodal distribution of cluster integrated colours...
Globular cluster systems (GCS) frequently show a bi-modal distribution of the cluster integrated col...
A large number of early-type galaxies are now known to possess blue and red subpopulations of globul...
A large number of early-type galaxies are now known to possess blue and red subpopulations of globul...
Original paper can be found at: http://www.astrosociety.org/pubs/cs/286.html--Copyright Astronomical...
We present Gemini griz' photometry for 521 globular cluster (GC) candidates in a 5.5 × 5.5 arcmin2 f...